7
Couplings Between Changes in the
Climate System and Biogeochemistry
Coordinating Lead Authors:
Kenneth L. Denman (Canada), Guy Brasseur (USA, Germany)
Lead Authors:
Amnat Chidthaisong (Thailand), Philippe Ciais (France), Peter M. Cox (UK), Robert E. Dickinson (USA), Didier Hauglustaine (France),
Christoph Heinze (Norway, Germany), Elisabeth Holland (USA), Daniel Jacob (USA, France), Ulrike Lohmann (Switzerland),
Srikanthan Ramachandran (India), Pedro Leite da Silva Dias (Brazil), Steven C. Wofsy (USA), Xiaoye Zhang (China)
Contributing Authors:
D. Archer (USA), V. Arora (Canada), J. Austin (USA), D. Baker (USA), J.A. Berry (USA), R. Betts (UK), G. Bonan (USA),
P. Bousquet (France), J. Canadell (Australia), J. Christian (Canada), D.A. Clark (USA), M. Dameris (Germany), F. Dentener (EU),
D. Easterling (USA), V. Eyring (Germany), J. Feichter (Germany), P. Friedlingstein (France, Belgium), I. Fung (USA), S. Fuzzi (Italy),
S. Gong (Canada), N. Gruber (USA, Switzerland), A. Guenther (USA), K. Gurney (USA), A. Henderson-Sellers (Switzerland), J. House (UK),
A. Jones (UK), C. Jones (UK), B. Kärcher (Germany), M. Kawamiya (Japan), K. Lassey (New Zealand), C. Le Quéré (UK, France, Canada),
C. Leck (Sweden), J. Lee-Taylor (USA, UK), Y. Malhi (UK), K. Masarie (USA), G. McFiggans (UK), S. Menon (USA), J.B. Miller (USA),
P. Peylin (France), A. Pitman (Australia), J. Quaas (Germany), M. Raupach (Australia), P. Rayner (France), G. Rehder (Germany),
U. Riebesell (Germany), C. Rödenbeck (Germany), L. Rotstayn (Australia), N. Roulet (Canada), C. Sabine (USA), M.G. Schultz (Germany),
M. Schulz (France, Germany), S.E. Schwartz (USA), W. Steffen (Australia), D. Stevenson (UK), Y. Tian (USA, China), K.E. Trenberth (USA),
T. Van Noije (Netherlands), O. Wild (Japan, UK), T. Zhang (USA, China), L. Zhou (USA, China)
Review Editors:
Kansri Boonpragob (Thailand), Martin Heimann (Germany, Switzerland), Mario Molina (USA, Mexico)
This chapter should be cited as:
Denman, K.L., G. Brasseur, A. Chidthaisong, P. Ciais, P.M. Cox, R.E. Dickinson, D. Hauglustaine, C. Heinze, E. Holland, D. Jacob, U.
Lohmann, S Ramachandran, P.L. da Silva Dias, S.C. Wofsy and X. Zhang, 2007: Couplings Between Changes in the Climate System
and Biogeochemistry. In:
Climate Change 2007: The Physical Science Basis. Contribution of Working Group I to the Fourth Assessment
Report of the Intergovernmental Panel on Climate Change
[Solomon, S., D. Qin, M. Manning, Z. Chen, M. Marquis, K.B. Averyt, M.Tignor
and H.L. Miller (eds.)]. Cambridge University Press, Cambridge, United Kingdom and New York, NY, USA.
500
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Table of Contents
Executive Summary
.................................................... 501
7.1 Introduction
......................................................... 503
7.1.1 Terrestrial Ecosystems and Climate .................... 503
7.1.2 Ocean Ecosystems and Climate ......................... 503
7.1.3 Atmospheric Chemistry and Climate ................... 504
7.1.4 Aerosol Particles and Climate ............................. 504
7.1.5 Coupling the Biogeochemical Cycles with the
Climate
System
................................................... 504
7.2 The Changing Land Climate System
.......... 504
7.2.1 Introduction to Land Climate ............................... 504
7.2.2 Dependence of Land Processes and
Climate on Scale ................................................. 505
Box 7.1: Surface Energy and Water Balance
...................... 505
Box 7.2: Urban Effects on Climate
.................................... 506
7.2.3 Observational Basis for the Effects of
Land Surface on Climate ..................................... 507
7.2.4 Modelling the Coupling of Vegetation,
Moisture Availability, Precipitation and Surface
Temperature
......................................................... 509
7.2.5 Evaluation of Models Through
Intercomparison
................................................... 510
7.2.6 Linking Biophysical to Biogeochemical and
Ecohydrological
Components
............................. 511
7.3 The Carbon Cycle and the
Climate
System
................................................... 511
7.3.1 Overview of the Global Carbon Cycle ................. 511
7.3.2 The Contemporary Carbon Budget ..................... 517
7.3.3 Terrestrial Carbon Cycle Processes and
Feedbacks to Climate.......................................... 526
7.3.4 Ocean Carbon Cycle Processes and
Feedbacks to Climate.......................................... 528
Box 7.3: Marine Carbon Chemistry and
Ocean Acidifi cation
............................................ 529
7.3.5 Coupling Between the Carbon Cycle
and
Climate
......................................................... 533
7.4 Reactive Gases and the Climate
System
..................................................................... 539
7.4.1 Methane ............................................................... 539
Box 7.4: Effects of Climate Change on Air Quality
............... 540
7.4.2 Nitrogen
Compounds
.......................................... 544
7.4.3. Molecular Hydrogen ............................................ 547
7.4.4 Global
Tropospheric
Ozone
................................. 547
7.4.5. The Hydroxyl Radical........................................... 550
7.4.6 Stratospheric Ozone and Climate ....................... 553
7.5 Aerosol Particles and the Climate
System
.................................................................... 555
7.5.1 Aerosol Emissions and Burdens Affected
by Climatic Factors .............................................. 555
7.5.2 Indirect Effects of Aerosols on Clouds
and
Precipitation.................................................. 559
7.5.3 Effects of Aerosols and Clouds on Solar
Radiation at the Earth’s Surface .......................... 563
7.5.4 Effects of Aerosols on Circulation Patterns ......... 564
7.6 Concluding
Remarks
......................................... 566
Frequently Asked Question
FAQ 7.1:
Are the Increases in Atmospheric Carbon
Dioxide and Other Greenhouse Gases During the
Industrial Era Caused by Human Activities?
........... 512
References
........................................................................ 568
501
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Executive Summary
Emissions of carbon dioxide, methane, nitrous oxide and of
reactive gases such as sulphur dioxide, nitrogen oxides, carbon
monoxide and hydrocarbons, which lead to the formation
of secondary pollutants including aerosol particles and
tropospheric ozone, have increased substantially in response to
human activities. As a result, biogeochemical cycles have been
perturbed signi
fi
cantly. Nonlinear interactions between the
climate and biogeochemical systems could amplify (positive
feedbacks) or attenuate (negative feedbacks) the disturbances
produced by human activities.
The Land Surface and Climate
• Changes in the land surface (vegetation, soils, water)
resulting from human activities can affect regional
climate through shifts in radiation, cloudiness and surface
temperature.
• Changes in vegetation cover affect surface energy and
water balances at the regional scale, from boreal to tropical
forests. Models indicate increased boreal forest reduces
the effects of snow albedo and causes regional warming.
Observations and models of tropical forests also show
effects of changing surface energy and water balance.
• The impact of land use change on the energy and water
balance may be very signi
fi
cant for climate at regional
scales over time periods of decades or longer.
The Carbon Cycle and Climate
• Atmospheric carbon dioxide (CO
2
) concentration has
continued to increase and is now almost 100 ppm above
its pre-industrial level. The annual mean CO
2
growth
rate was signi
fi
cantly higher for the period from 2000 to
2005 (4.1 ± 0.1 GtC yr
–1
) than it was in the 1990s (3.2 ±
0.1 GtC yr
–1
). Annual emissions of CO
2
from fossil fuel
burning and cement production increased from a mean of
6.4 ± 0.4 GtC yr
–1
in the 1990s to 7.2 ± 0.3 GtC yr
–1
for
2000 to 2005.
1
•
Carbon dioxide cycles between the atmosphere, oceans and
land biosphere. Its removal from the atmosphere involves a
range of processes with different time scales. About 50% of
a CO
2
increase will be removed from the atmosphere within
30 years, and a further 30% will be removed within a few
centuries. The remaining 20% may stay in the atmosphere
for many thousands of years.
•
Improved estimates of ocean uptake of CO
2
suggest little
change in the ocean carbon sink of 2.2 ± 0.5 GtC yr
–1
between the 1990s and the
fi
rst
fi
ve years of the 21st
century. Models indicate that the fraction of fossil fuel
and cement emissions of CO
2
taken up by the ocean will
decline if atmospheric CO
2
continues to increase.
• Interannual and inter-decadal variability in the growth
rate of atmospheric CO
2
is dominated by the response
of the land biosphere to climate variations. Evidence
of decadal changes is observed in the net land carbon
sink, with estimates of 0.3 ± 0.9, 1.0 ± 0.6, and 0.9 ±
0.6 GtC yr
–1
for the 1980s, 1990s and 2000 to 2005 time
periods, respectively.
• A combination of techniques gives an estimate of the
fl
ux of CO
2
to the atmosphere from land use change of
1.6 (0.5 to 2.7) GtC yr
–1
for the 1990s. A revision of the
Third Assessment Report (TAR) estimate for the 1980s
downwards to 1.4 (0.4 to 2.3) GtC yr
–1
suggests little change
between the 1980s and 1990s, and continuing uncertainty
in the net CO
2
emissions due to land use change.
•
Fires, from natural causes and human activities, release to
the atmosphere considerable amounts of radiatively and
photochemically active trace gases and aerosols. If
fi
re
frequency and extent increase with a changing climate, a
net increase in CO
2
emissions is expected during this
fi
re
regime shift.
• There is yet no statistically signi
fi
cant trend in the CO
2
growth rate as a fraction of fossil fuel plus cement emissions
since routine atmospheric CO
2
measurements began in
1958. This ‘airborne fraction’ has shown little variation
over this period.
• Ocean
CO
2
uptake has lowered the average ocean pH
(increased acidity) by approximately 0.1 since 1750.
Consequences for marine ecosystems may include reduced
calci
fi
cation by shell-forming organisms, and in the longer
term, the dissolution of carbonate sediments.
• The
fi
rst-generation coupled climate-carbon cycle models
indicate that global warming will increase the fraction
of anthropogenic CO
2
that remains in the atmosphere.
This positive climate-carbon cycle feedback leads to an
additional increase in atmospheric CO
2
concentration of
20 to 224 ppm by 2100, in models run under the IPCC
(2000) Special Report on Emission Scenarios (SRES) A2
emissions scenario.
Reactive Gases and Climate
•
Observed increases in atmospheric methane concentration,
compared with pre-industrial estimates, are directly linked
to human activity, including agriculture, energy production,
1
The uncertainty ranges given here and especially in Tables 7.1 and 7. 2 are the authors’ estimates of the
likely
(66%) range for each term based on their assessment of the
currently available studies. There are not enough comparable studies to enable estimation of a
very
likely
(90%) range for all the main terms in the carbon cycle budget.
502
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
waste management and biomass burning. Constraints
from methyl chloroform observations show that there
have been no signi
fi
cant trends in hydroxyl radical (OH)
concentrations, and hence in methane removal rates, over
the past few decades (see Chapter 2). The recent slowdown
in the growth rate of atmospheric methane since about
1993 is thus
likely
due to the atmosphere approaching an
equilibrium during a period of near-constant total emissions.
However, future methane emissions from wetlands are
likely
to increase in a warmer and wetter climate, and to
decrease in a warmer and drier climate.
• No long-term trends in the tropospheric concentration
of OH are expected over the next few decades due to
offsetting effects from changes in nitric oxides (NO
x
),
carbon monoxide, organic emissions and climate change.
Interannual variability of OH may continue to affect the
variability of methane.
• New model estimates of the global tropospheric ozone
budget indicate that input of ozone from the stratosphere
(approximately 500 Tg yr
–1
) is smaller than estimated in the
TAR (770 Tg yr
–1
), while the photochemical production and
destruction rates (approximately 5,000 and 4,500 Tg yr
–1
respectively) are higher than estimated in the TAR (3,400
and 3,500 Tg yr
–1
). This implies greater sensitivity of ozone
to changes in tropospheric chemistry and emissions.
• Observed increases in NO
x
and nitric oxide emissions,
compared with pre-industrial estimates, are
very
likely
directly linked to ‘acceleration’ of the nitrogen cycle
driven by human activity, including increased fertilizer use,
intensi
fi
cation of agriculture and fossil fuel combustion.
• Future climate change may cause either an increase or a
decrease in background tropospheric ozone, due to the
competing effects of higher water vapour and higher
stratospheric input; increases in regional ozone pollution
are expected due to higher temperatures and weaker
circulation.
• Future climate change may cause signi
fi
cant air quality
degradation by changing the dispersion rate of pollutants,
the chemical environment for ozone and aerosol generation
and the strength of emissions from the biosphere,
fi
res and
dust. The sign and magnitude of these effects are highly
uncertain and will vary regionally.
•
The future evolution of stratospheric ozone, and therefore
its recovery following its destruction by industrially
manufactured halocarbons, will be in
fl
uenced by
stratospheric cooling and changes in the atmospheric
circulation resulting from enhanced CO
2
concentrations.
With a possible exception in the polar lower stratosphere
where colder temperatures favour ozone destruction by
chlorine activated on polar stratospheric cloud particles,
the expected cooling of the stratosphere should reduce
ozone depletion and therefore enhance the ozone column
amounts.
Aerosol Particles and Climate
• Sulphate aerosol particles are responsible for globally
averaged temperatures being lower than expected from
greenhouse gas concentrations alone.
• Aerosols affect radiative
fl
uxes by scattering and absorbing
solar radiation (direct effect, see Chapter 2). They also
interact with clouds and the hydrological cycle by acting as
cloud condensation nuclei (CCN) and ice nuclei. For a given
cloud liquid water content, a larger number of CCN increases
cloud albedo (indirect cloud albedo effect) and reduces the
precipitation ef
fi
ciency (indirect cloud lifetime effect), both of
which are
likely
to result in a reduction of the global, annual
mean net radiation at the top of the atmosphere. However,
these effects may be partly offset by evaporation of cloud
droplets due to absorbing aerosols (semi-direct effect) and/or
by more ice nuclei (glaciation effect).
• The estimated total aerosol effect is lower than in TAR
mainly due to improvements in cloud parametrizations, but
large uncertainties remain.
• The radiative forcing resulting from the indirect cloud
albedo effect was estimated in Chapter 2 as –0.7 W m
–2
with a 90% con
fi
dence range of –0.3 to –1.8 W m
–2
.
Feedbacks due to the cloud lifetime effect, semi-direct
effect or aerosol-ice cloud effects can either enhance or
reduce the cloud albedo effect. Climate models estimate
the sum of all aerosol effects (total indirect plus direct) to
be –1.2 W m
–2
with a range from –0.2 to –2.3 W m
–2
in the
change in top-of-the-atmosphere net radiation since pre-
industrial times, whereas inverse estimates constrain the
indirect aerosol effect to be between –0.1 and –1.7 W m
–2
(see Chapter 9).
•
The magnitude of the total aerosol effect on precipitation
is more uncertain, with model results ranging from almost
no change to a decrease of 0.13 mm day
–1
. Decreases in
precipitation are larger when the atmospheric General
Circulation Models are coupled to mixed-layer ocean
models where the sea surface temperature and, hence, the
evaporation is allowed to vary.
• Deposition of dust particles containing limiting nutrients
can enhance photosynthetic carbon
fi
xation on land and in
the oceans. Climate change is likely to affect dust sources.
• Since the TAR, advances have been made to link the
marine and terrestrial biospheres with the climate system
via the aerosol cycle. Emissions of aerosol precursors from
vegetation and from the marine biosphere are expected to
respond to climate change.
503
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.1 Introduction
The Earth’s climate is determined by a number of complex
connected physical, chemical and biological processes
occurring in the atmosphere, land and ocean. The radiative
properties of the atmosphere, a major controlling factor of the
Earth’s climate, are strongly affected by the biophysical state
of the Earth’s surface and by the atmospheric abundance of a
variety of trace constituents. These constituents include long-
lived greenhouse gases (LLGHGs) such as carbon dioxide
(CO
2
), methane (CH
4
) and nitrous oxide (N
2
O), as well as
other radiatively active constituents such as ozone and different
types of aerosol particles. The composition of the atmosphere
is determined by processes such as natural and anthropogenic
emissions of gases and aerosols, transport at a variety of scales,
chemical and microphysical transformations, wet scavenging
and surface uptake by the land and terrestrial ecosystems, and
by the ocean and its ecosystems. These processes and, more
generally the rates of biogeochemical cycling, are affected by
climate change, and involve interactions between and within the
different components of the Earth system. These interactions
are generally nonlinear and may produce negative or positive
feedbacks to the climate system.
An important aspect of climate research is to identify potential
feedbacks and assess if such feedbacks could produce large
and undesired responses to perturbations resulting from human
activities. Studies of past climate evolution on different time scales
can elucidate mechanisms that could trigger nonlinear responses to
external forcing. The purpose of this chapter is to identify the major
biogeochemical feedbacks of signi
fi
cance to the climate system,
and to assess current knowledge of their magnitudes and trends.
Speci
fi
cally, this chapter will examine the relationships between
the physical climate system and the land surface, the carbon cycle,
chemically reactive atmospheric gases and aerosol particles. It also
presents the current state of knowledge on budgets of important
trace gases. Large uncertainties remain in many issues discussed
in this chapter, so that quantitative estimates of the importance of
the coupling mechanisms discussed in the following sections are
not always available. In addition, regional differences in the role
of some cycles and the complex interactions between them limit
our present ability to provide a simple quantitative description of
the interactions between biogeochemical processes and climate
change.
7.1.1
Terrestrial Ecosystems and Climate
The terrestrial biosphere interacts strongly with the
climate, providing both positive and negative feedbacks due to
biogeophysical and biogeochemical processes. Some of these
feedbacks, at least on a regional basis, can be large. Surface
climate is determined by the balance of
fl
uxes, which can be
changed by radiative (e.g., albedo) or non-radiative (e.g., water
cycle related processes) terms. Both radiative and non-radiative
terms are controlled by details of vegetation. High-latitude
climate is strongly in
fl
uenced by snow albedo feedback, which
is drastically reduced by the darkening effect of vegetation.
In semi-arid tropical systems, such as the Sahel or northeast
Brazil, vegetation exerts both radiative and hydrological
feedbacks. Surface climate interacts with vegetation cover,
biomes, productivity, respiration of vegetation and soil, and
fi
res, all of which are important for the carbon cycle. Various
processes in terrestrial ecosystems in
fl
uence the
fl
ux of carbon
between land and the atmosphere. Terrestrial ecosystem
photosynthetic productivity changes in response to changes
in temperature, precipitation, CO
2
and nutrients. If climate
becomes more favourable for growth (e.g., increased rainfall in
a semi-arid system), productivity increases, and carbon uptake
from the atmosphere is enhanced. Organic carbon compounds
in soils, originally derived from plant material, are respired
(i.e., oxidized by microbial communities) at different rates
depending on the nature of the compound and on the microbial
communities; the aggregate rate of respiration depends on
soil temperature and moisture. Shifts in ecosystem structure
in response to a changing climate can alter the partitioning of
carbon between the atmosphere and the land surface. Migration
of boreal forest northward into tundra would initially lead to an
increase in carbon storage in the ecosystem due to the larger
biomass of trees than of herbs and shrubs, but over a longer
time (e.g., centuries), changes in soil carbon would need to be
considered to determine the net effect. A shift from tropical
rainforest to savannah, on the other hand, would result in a net
fl
ux of carbon from the land surface to the atmosphere.
7.1.2
Ocean Ecosystems and Climate
The functioning of ocean ecosystems depends strongly on
climatic conditions including near-surface density strati
fi
cation,
ocean circulation, temperature, salinity, the wind
fi
eld and
sea ice cover. In turn, ocean ecosystems affect the chemical
composition of the atmosphere (e.g. CO
2
, N
2
O, oxygen (O
2
),
dimethyl sulphide (DMS) and sulphate aerosol). Most of these
components are expected to change with a changing climate
and high atmospheric CO
2
conditions. Marine biota also
in
fl
uence the near-surface radiation budget through changes
in the marine albedo and absorption of solar radiation (bio-
optical heating). Feedbacks between marine ecosystems and
climate change are complex because most involve the ocean’s
physical responses and feedbacks to climate change. Increased
surface temperatures and strati
fi
cation should lead to increased
photosynthetic
fi
xation of CO
2
, but associated reductions in
vertical mixing and overturning circulation may decrease the
return of required nutrients to the surface ocean and alter the
vertical export of carbon to the deeper ocean. The sign of the
cumulative feedback to climate of all these processes is still
unclear. Changes in the supply of micronutrients required for
photosynthesis, in particular iron, through dust deposition to the
ocean surface can modify marine biological production patterns.
Ocean acidi
fi
cation due to uptake of anthropogenic CO
2
may
lead to shifts in ocean ecosystem structure and dynamics, which
may alter the biological production and export from the surface
ocean of organic carbon and calcium carbonate (CaCO
3
).
504
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
release to the atmosphere depends on climatic factors. In many
areas of the Earth, large amounts of SO
4
particles are produced
as a result of human activities (e.g., coal burning). With an
elevated atmospheric aerosol load, principally in the Northern
Hemisphere (NH), it is likely that the temperature increase
during the last century has been smaller than the increase that
would have resulted from radiative forcing by greenhouse
gases alone. Other indirect effects of aerosols on climate
include the evaporation of cloud particles through absorption
of solar radiation by soot, which in this case provides a positive
warming effect. Aerosols (i.e., dust) also deliver nitrogen (N),
phosphorus and iron to the Earth’s surface; these nutrients could
increase uptake of CO
2
by marine and terrestrial ecosystems.
7.1.5
Coupling the Biogeochemical Cycles with the
Climate System
Models that attempt to perform reliable projections of future
climate changes should account explicitly for the feedbacks
between climate and the processes that determine the
atmospheric concentrations of greenhouse gases, reactive gases
and aerosol particles. An example is provided by the interaction
between the carbon cycle and climate. It is well established that
the level of atmospheric CO
2
, which directly in
fl
uences the
Earth’s temperature, depends critically on the rates of carbon
uptake by the ocean and the land, which are also dependent
on climate. Climate models that include the dynamics of the
carbon cycle suggest that the overall effect of carbon-climate
interactions is a positive feedback. Hence predicted future
atmospheric CO
2
concentrations are therefore higher (and
consequently the climate warmer) than in models that do not
include these couplings. As understanding of the role of the
biogeochemical cycles in the climate system improves, they
should be explicitly represented in climate models. The present
chapter assesses the current understanding of the processes
involved and highlights the role of biogeochemical processes
in the climate system.
7.2 The Changing Land Climate System
7.2.1
Introduction to Land Climate
The land surface relevant to climate consists of the terrestrial
biosphere, that is, the fabric of soils, vegetation and other
biological components, the processes that connect them and
the carbon, water and energy they store. This section addresses
from a climate perspective the current state of understanding of
the land surface, setting the stage for consideration of carbon
and other biogenic processes linked to climate. The land climate
consists of ‘internal’ variables and ‘external’ drivers, including
the various surface energy, carbon and moisture stores, and
their response to precipitation, incoming radiation and near-
surface atmospheric variables. The drivers and response
variables change over various temporal and spatial scales.
7.1.3 Atmospheric Chemistry and Climate
Interactions between climate and atmospheric oxidants,
including ozone, provide important coupling mechanisms in
the Earth system. The concentration of tropospheric ozone
has increased substantially since the pre-industrial era,
especially in polluted areas of the world, and has contributed
to radiative warming. Emissions of chemical ozone precursors
(carbon monoxide, CH
4
, non-methane hydrocarbons, nitrogen
oxides) have increased as a result of larger use of fossil fuel,
more frequent biomass burning and more intense agricultural
practices. The atmospheric concentration of pre-industrial
tropospheric ozone is not accurately known, so that the resulting
radiative forcing cannot be accurately determined, and must
be estimated from models. The decrease in concentration of
stratospheric ozone in the 1980s and 1990s due to manufactured
halocarbons (which produced a slight cooling) has slowed
down since the late 1990s. Model projections suggest a slow
steady increase over the next century, but continued recovery
could be affected by future climate change. Recent changes in
the growth rate of atmospheric CH
4
and in its apparent lifetime
are not well understood, but indications are that there have
been changes in source strengths. Nitrous oxide continues to
increase in the atmosphere, primarily as a result of agricultural
activities. Changes in atmospheric chemical composition that
could result from climate changes are even less well quanti
fi
ed.
Photochemical production of the hydroxyl radical (OH), which
ef
fi
ciently destroys many atmospheric compounds, occurs
in the presence of ozone and water vapour, and should be
enhanced in an atmosphere with increased water vapour, as
projected under future global warming. Other chemistry-related
processes affected by climate change include the frequency of
lightning
fl
ashes in thunderstorms (which produce nitrogen
oxides), scavenging mechanisms that remove soluble species
from the atmosphere, the intensity and frequency of convective
transport events, the natural emissions of chemical compounds
(e.g., biogenic hydrocarbons by the vegetation, nitrous and
nitric oxide by soils, DMS from the ocean) and the surface
deposition on molecules on the vegetation and soils. Changes
in the circulation and speci
fi
cally the more frequent occurrence
of stagnant air events in urban or industrial areas could enhance
the intensity of air pollution events. The importance of these
effects is not yet well quanti
fi
ed.
7.1.4
Aerosol Particles and Climate
Atmospheric aerosol particles modify Earth’s radiation
budget by absorbing and scattering incoming solar radiation.
Even though some particle types may have a warming effect,
most aerosol particles, such as sulphate (SO
4
) aerosol particles,
tend to cool the Earth surface by scattering some of the incoming
solar radiation back to space. In addition, by acting as cloud
condensation nuclei, aerosol particles affect radiative properties
of clouds and their lifetimes, which contribute to additional
surface cooling. A signi
fi
cant natural source of sulphate is DMS,
an organic compound whose production by phytoplankton and
505
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
This variation in time and space can be at least as important as
averaged quantities. The response variables and drivers for the
terrestrial system can be divided into biophysical, biological,
biogeochemical and human processes. The present biophysical
viewpoint emphasizes the response variables that involve the
stores of energy and water and the mechanisms coupling these
terms to the atmosphere. The exchanges of energy and moisture
between the atmosphere and land surface (Boxes 7.1 and 7.2)
are driven by radiation, precipitation and the temperature,
humidity and winds of the overlying atmosphere. Determining
how much detail to include to achieve an understanding of the
system is not easy: many choices can be made and more detail
becomes necessary when more processes are to be addressed.
7.2.2 Dependence of Land Processes and Climate
on Scale
7.2.2.1
Multiple Scales are Important
Temporal variability ranges from the daily and weather time
scales to annual, interannual, and decadal or longer scales: the
amplitudes of shorter time scales change with long-term changes
from global warming. The land climate system has controls on
amplitudes of variables on all these time scales, varying with
season and geography. For example, Trenberth and Shea (2005)
evaluate from climatic observations the correlation between
surface air temperature and precipitation, and
fi
nd a strong
r
> 0.3) positive correlation over most winter land areas (i.e.,
poleward of 40°N) but a strong (|
r
| > 0.3) negative correlation
over much of summer and tropical land. These differences result
from competing feedbacks with the water cycle. On scales
large enough that surface temperatures control atmospheric
temperatures, the atmosphere will hold more water vapour and
may provide more precipitation with warmer temperatures. Low
clouds strongly control surface temperatures, especially in cold
regions where they make the surface warmer. In warm regions
without precipitation, the land surface can become warmer
because of lack of evaporation, or lack of clouds. Although
a drier surface will become warmer from lack of evaporative
cooling, more water can evaporate from a moist surface if the
temperature is warmer (see Box 7.1).
7.2.2.2
Spatial Dependence
Drivers of the land climate system have larger effects
at regional and local scales than on global climate, which is
controlled primarily by processes of global radiation balance.
Myhre et al. (2005) point out that the albedo of agricultural
systems may be only slightly higher than that of forests and
estimate that the impact since pre-agricultural times of land use
Box 7.1: Surface Energy and Water Balance
The land surface on average is heated by net radiation balanced by exchanges with the atmosphere of sensible and latent heat,
known as the ‘surface energy balance’. Sensible heat is the energy carried by the atmosphere in its temperature and latent heat is the
energy lost from the surface by evaporation of surface water. The latent heat of the water vapour is converted to sensible heat in the
atmosphere through vapour condensation and this condensed water is returned to the surface through precipitation.
The surface also has a ‘surface water balance’. Water coming to the surface from precipitation is eventually lost either through water
vapour fl ux or by runoff . The latent heat fl ux (or equivalently water vapour fl ux) under some conditions can be determined from the
energy balance. For a fi xed amount of net surface radiation, if the sensible heat fl ux goes up, the latent fl ux will go down by the same
amount. Thus, if the ratio of sensible to latent heat fl ux depends only on air temperature, relative humidity and other known factors,
the fl ux of water vapour from the surface can be found from the net radiative energy at the surface. Such a relationship is most read-
ily obtained when water removal (evaporation from soil or transpiration by plants) is not limited by availability of water. Under these
conditions, the increase of water vapour concentration with temperature increases the relative amount of the water fl ux as does low
relative humidity. Vegetation can prolong the availability of soil water through the extent of its roots and so increase the latent heat
fl ux but also can resist movement through its leaves, and so shift the surface energy fl uxes to a larger fraction carried by the sensible
heat fl ux. Fluxes to the atmosphere modify atmospheric temperatures and humidity and such changes feed back to the fl uxes. Storage
and the surface can also be important at short time scales, and horizontal transports can be important at smaller spatial scales.
If a surface is too dry to exchange much water with the atmosphere, the water returned to the atmosphere should be on average
not far below the incident precipitation, and radiative energy beyond that needed for evaporating this water will heat the surface.
Under these circumstances, less precipitation and hence less water vapour fl ux will make the surface warmer. Reduction of cloudiness
from the consequently warmer and drier atmosphere may act as a positive feedback to provide more solar radiation. A locally moist
area (such as an oasis or pond), however, would still evaporate according to energy balance with no water limitation and thus should
increase its evaporation under such warmer and drier conditions.
Various feedbacks coupling the surface to the atmosphere may work in opposite directions and their relative importance may
depend on season and location as well as on temporal and spatial scales. A moister atmosphere will commonly be cloudier making
the surface warmer in a cold climate and cooler in a warm climate. The warming of the atmosphere by the surface may reduce its rela-
tive humidity and reduce precipitation as happens over deserts. However, it can also increase the total water held by the atmosphere,
which may lead to increased precipitation as happens over the tropical oceans.
506
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
conversion to agriculture on global radiative forcing has been
only –0.09 W m
–2
, that is, about 5% of the warming contributed
by CO
2
since pre-industrial times (see Chapter 2 for a more
comprehensive review of recent estimates of land surface
albedo change). Land comprises only about 30% of the Earth’s
surface, but it can have the largest effects on the re
fl
ection of
global solar radiation in conjunction with changes in ice and
snow cover, and the shading of the latter by vegetation.
At a regional scale and at the surface, additional more
localised and shorter time-scale processes besides radiative
forcing can affect climate in other ways, and possibly be of
comparable importance to the effects of the greenhouse gases.
Changes over land that modify its evaporative cooling can
cause large changes in surface temperature, both locally and
regionally (see Boxes 7.1, 7.2). How this change feeds back
to precipitation remains a major research question. Land has a
strong control on the vertical distribution of atmospheric heating.
It determines how much of the radiation delivered to land goes
into warming the near-surface atmosphere compared with how
much is released as latent heat fuelling precipitation at higher
levels. Low clouds are normally closely coupled to the surface
and over land can be signi
fi
cantly changed by modi
fi
cations
of surface temperature or moisture resulting from changes in
land properties. For example, Chagnon et al. (2004)
fi
nd a large
increase in boundary layer clouds in the Amazon in areas of
partial deforestation (also, e.g., Durieux et al., 2003; Ek and
Holtslag, 2004). Details of surface properties at scales as small
as a few kilometres can be important for larger scales. Over
some fraction of moist soils, water tables can be high enough
to be hydrologically connected to the rooting zone, or reach the
surface as in wetlands (e.g., Koster et al., 2000; Marani et al.,
2001; Milly and Shmakin, 2002; Liang et al., 2003; Gedney and
Cox, 2003).
The consequences of changes in atmospheric heating from
land changes at a regional scale are similar to those from ocean
temperature changes such as from El Niño, potentially producing
patterns of reduced or increased cloudiness and precipitation
elsewhere to maintain global energy balance. Attempts have
been made to
fi
nd remote adjustments (e.g., Avissar and
Werth, 2005). Such adjustments may occur in multiple ways,
and are part of the dynamics of climate models. The locally
warmer temperatures can lead to more rapid vertical decreases
of atmospheric temperature so that at some level overlying
temperature is lower and radiates less. The net effect of such
compensations is that averages over larger areas or longer time
scales commonly will give smaller estimates of change. Thus,
such regional changes are better described by local and regional
metrics or at larger scales by measures of change in spatial
and temporal variability rather than simply in terms of a mean
global quantity.
7.2.2.3 Daily and Seasonal Variability
Diurnal and seasonal variability result directly from the
temporal variation of the solar radiation driver. Large-scale
changes in climate variables are of interest as part of the
observational record of climate changes (Chapter 3). Daytime
during the warm season produces a thick layer of mixed air with
temperature relatively insensitive to perturbations in daytime
radiative forcing. Nighttime and high-latitude winter surface
temperatures, on the other hand, are coupled by mixing to only
a thin layer of atmosphere, and can be more readily altered by
changes in atmospheric downward thermal radiation. Thus,
land is more sensitive to changes in radiative drivers under cold
stable conditions and weak winds than under warm unstable
conditions. Winter or nighttime temperatures (hence diurnal
temperature range) are strongly correlated with downward
longwave radiation (e.g., Betts, 2006; Dickinson et al., 2006);
consequently, average surface temperatures may change (e.g.,
Pielke and Matsui, 2005) with a change in downward longwave
radiation.
Modi
fi
cation of downward longwave radiation by changes
in clouds can affect land surface temperatures. Qian and Giorgi
(2000) discussed regional aerosol effects, and noted a reduction
in the diurnal temperature range of –0.26°C per decade over
Sichuan China. Huang et al. (2006) model the growth of sulphate
aerosols and their interactions with clouds in the context of a
RCM, and
fi
nd over southern China a decrease in the diurnal
temperature range comparable with that observed by Zhou
et al. (2004) and Qian and Giorgi. They show the nighttime
temperature change to be a result of increased nighttime
cloudiness and hence downward longwave radiation connected
to the increase in aerosols.
Box 7.2: Urban Effects on Climate
If the properties of the land surface are changed locally,
the surface net radiation and the partitioning between latent
and sensible fl uxes (Box 7.1) may also change, with conse-
quences for temperatures and moisture storage of the sur-
face and near-surface air. Such changes commonly occur to
meet human needs for agriculture, housing, or commerce
and industry. The consequences of urban development may
be especially signifi cant for local climates. However, urban
development may have diff erent features in diff erent parts
of an urban area and between geographical regions.
Some common modifi cations are the replacement of
vegetation by impervious surfaces such as roads or the con-
verse development of dry surfaces into vegetated surfaces
by irrigation, such as lawns and golf courses. Buildings cover
a relatively small area but in urban cores may strongly modify
local wind fl ow and surface energy balance (Box 7.1). Besides
the near-surface eff ects, urban areas can provide high con-
centrations of aerosols with local or downwind impacts on
clouds and precipitation. Change to dark dry surfaces such
as roads will generally increase daytime temperatures and
lower humidity while irrigation will do the opposite. Chang-
es at night may depend on the retention of heat by buildings
and can be exacerbated by the thinness of the layer of atmo-
sphere connected to the surface by mixing of air. Chapter 3
further addresses urban eff ects.
507
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
In moist warm regions, large changes are possible in the
fraction of energy going into water
fl
uxes, for example, by
changes in vegetation cover or precipitation, and hence in soil
moisture. Bonan (2001) and Oleson et al. (2004) indicate that
conversion of mid-latitude forests to agriculture could cause a
daytime cooling. This cooling is apparently a result of higher
albedo and increased transpiration. Changes in re
fl
ected solar
radiation due to changing vegetation, hence feedbacks, are most
pronounced in areas with vegetation underlain by snow or light-
coloured soil. Seasonal and diurnal precipitation cycles can be
pronounced. Climate models simulate the diurnal precipitation
cycle but apparently not yet very well (e.g., Collier and
Bowman, 2004). Betts (2004) reviews how the diurnal cycle
of tropical continental precipitation is linked to land surface
fl
uxes and argues that errors in a model can feed back to model
dynamics with global impacts.
7.2.2.4 Coupling of Precipitation Intensities to Leaf
Water – An Issue Involving both Temporal and
Spatial Scales
The bulk of the water exchanged with the atmosphere is
stored in the soil until taken up by plant roots, typically weeks
later. However, the rapidity of evaporation of the near-surface
stores allows plant uptake and evaporation to be of comparable
importance for surface water and energy balances. (Dickinson
et al., 2003, conclude that feedbacks between surface moisture
and precipitation may act differently on different time scales).
Evaporation from the fast reservoirs acts primarily as a surface
energy removal mechanism. Leaves initially intercept much of
the precipitation over vegetation, and a signi
fi
cant fraction of this
leaf water re-evaporates in an hour or less. This loss reduces the
amount of water stored in the soil for use by plants. Its magnitude
depends inversely on the intensity of the precipitation, which can
be larger at smaller temporal and spatial scales. Modelling
results can be wrong either through neglect of or through
exaggeration of the magnitude of the fast time-scale
moisture stores.
Leaf water evaporation may have little effect on the
determination of monthly evapotranspiration (e.g., as
found in the analysis of Desborough, 1999) but may
still produce important changes in temperature and
precipitation. Pitman et al. (2004), in a coupled study
with land con
fi
gurations of different complexity, were
unable to
fi
nd any impacts on atmospheric variability,
but Bagnoud et al. (2005) found that precipitation and
temperature extremes were affected. Some studies that
change the intensity of precipitation
fi
nd a very large
impact from leaf water. For example, Wang and Eltahir
(2000) studied the effect of including more realistic
precipitation intensity compared to the uniform intensity
of a climate model. Hahmann (2003) used another model
to study this effect. Figure 7.1 compares their tropical
results (Wang and Eltahir over equatorial Africa and
Hahmann over equatorial Amazon). The model of Wang
and Eltahir shows that more realistic precipitation greatly
increases runoff whereas Hahmann shows that it reduces runoff.
It has not been determined whether these contradictory results
are more a consequence of model differences or of differences
between the climates of the two continents, as Hahmann
suggests.
7.2.3
Observational Basis for the Effects of Land
Surface on Climate
7.2.3.1
Vegetative Controls on Soil Water and its Return
Flux to the Atmosphere
Scanlon et al. (2005) provide an example of how soil
moisture can depend on vegetation. They monitored soil
moisture in the Nevada desert with lysimeters either including
or excluding vegetation and for a multi-year period that included
times of anomalously strong precipitation. Without vegetation,
much of the moisture penetrated deeply, had a long lifetime and
became available for recharge of deep groundwater, whereas
for the vegetated plot, the soil moisture was all transpired. In
the absence of leaves, forests in early spring also appear as
especially dry surfaces with consequent large sensible
fl
uxes
that mix the atmosphere to a great depth (e.g., Betts et al., 2001).
Increased water
fl
uxes with spring green-up are observed in
terms of a reduction in temperature. Trees in the Amazon can
have the largest water
fl
uxes in the dry season by development
of deep roots (Da Rocha et al., 2004; Quesada et al., 2004).
Forests can also retard
fl
uxes through control by their leaves.
Such control by vegetation of water
fl
uxes is most pronounced
for taller or sparser vegetation in cooler or drier climates, and
from leaves that are sparse or exert the strongest resistance
to water movement. The boreal forest, in particular, has been
characterised as a ‘green desert’ because of its small release of
water to the atmosphere (Gamon et al., 2003).
Figure 7.1.
Rainfall, runoff and evapotranspiration derived from climate simulation
results of Hahmann (H; 2004) and Wang and Eltahir (W; 2000). Hahmann’s results are for
the Amazon centred on the equator, and Wang and Eltahir’s for Africa at the equator. Both
studies examined the differences between ‘uniform’ precipitation over a model grid square
and ‘variable’ precipitation (added to about 10% of the grid square). Large differences are
seen between the two cases in the two studies: a large reduction in precipitation is seen in
the Hahmann variable case relative to the uniform case, whereas an increase is seen for
the Wang and Eltahir variable case. The differences are even greater for runoff: Hahmann’s
uniform case runoff is three times as large as the variable case, whereas Wang and Eltahir
have almost no runoff for their uniform case.
508
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.2.3.2
Land Feedback to Precipitation
Findell and Eltahir (2003) examine the correlation between
early morning near-surface humidity over the USA and an index
of the likelihood of precipitation occurrence. They identify
different geographical regions with positive, negative or little
correlation. Koster et al. (2003) and Koster and Suarez (2004)
show during summer over the USA, and all land 30°N to 60°N,
respectively, a signi
fi
cant correlation of monthly precipitation
with that of prior months. They further show that their model only
reproduces this correlation if soil moisture feedback is allowed to
affect precipitation. Additional observational evidence for such
feedback is noted by D’Odorico and Porporato (2004) in support
of a simpli
fi
ed model of precipitation soil moisture coupling (see,
e.g., Salvucci et al., 2002, for support of the null hypothesis of
no coupling). Liebmann and Marengo (2001) point out that the
interannual variation of precipitation over the Amazon is largely
controlled by the timing of the onset and end of the rainy season.
Li and Fu (2004) provide evidence that onset time of the rainy
season is strongly dependent on transpiration by vegetation
during the dry season. Previous modelling and observational
studies have also suggested that Amazon deforestation should
lead to a longer dry season. Fu and Li (2004) further argue from
observations that removal of tropical forest reduces surface
moisture
fl
uxes, and that such land use changes should contribute
to a lengthening of the Amazon dry season. Durieux et al. (2003)
fi
nd more rainfall in the deforested area in the wet season and a
reduction of the dry season precipitation over deforested regions
compared with forested areas. Negri et al. (2004) obtain an
opposite result (although their result is consistent with Durieux
during the wet season).
7.2.3.3 Properties
Affecting
Radiation
Albedo (the fraction of re
fl
ected solar radiation) and
emissivity (the ratio of thermal radiation to that of a black
body) are important variables for the radiative balance.
Surfaces that have more or taller vegetation are commonly
darker than are those with sparse or shorter vegetation. With
sparse vegetation, the net surface albedo also depends on the
albedo of the underlying surfaces, especially if snow or a light-
coloured soil. A large-scale transformation of tundra to shrubs,
possibly connected to warmer temperatures over the last few
decades, has been observed (e.g., Chapin et al., 2005). Sturm et
al. (2005) report on winter and melt season observations of how
varying extents of such shrubs can modify surface albedo. New
satellite data show the importance of radiation heterogeneities
at the plot scale for the determination of albedo and the solar
radiation used for photosynthesis, and appropriate modelling
concepts to incorporate the new data are being advanced (e.g.,
Yang and Friedl, 2003; Niu and Yang, 2004; Wang, 2005; Pinty
et al., 2006).
7.2.3.4
Improved Global and Regional Data
Speci
fi
cation of land surface properties has improved through
new, more accurate global satellite observations. In particular,
satellite observations have provided albedos of soils in non-
vegetated regions (e.g., Tsvetsinskaya et al., 2002; Ogawa and
Schmugge, 2004; Z. Wang, et al., 2004; Zhou et al., 2005) and
their emissivities (Zhou et al., 2003a,b). They also constrain
model-calculated albedos in the presence of vegetation (Oleson
et al., 2003) and vegetation underlain by snow (Jin et al., 2002),
and help to de
fi
ne the in
fl
uence of leaf area on albedo (Tian
et al., 2004). Precipitation data sets combining rain gauge and
satellite observations (Chen et al., 2002; Adler et al., 2003) are
providing diagnostic constraints for climate modelling, as are
observations of runoff (Dai and Trenberth, 2002; Fekete et al.,
2002).
7.2.3.5 Field Observational Programs
New and improved local site observational constraints
collectively describe the land processes that need to be modelled.
The largest recent such activity has been the Large-Scale
Biosphere-Atmosphere Experiment in Amazonia (LBA) project
(Malhi et al., 2002; Silva Dias et al., 2002). Studies within LBA
have included physical climate at all scales, carbon and nutrient
dynamics and trace gas
fl
uxes. The physical climate aspects are
reviewed here. Goncalves et al. (2004) discuss the importance of
incorporating land cover heterogeneity. Da Rocha et al. (2004)
and Quesada et al. (2004) quantify water and energy budgets
for a forested and a savannah site, respectively. Dry season
evapotranspiration for the savannah averaged 1.6 mm day
–1
compared with 4.9 mm day
–1
for the forest. Both ecosystems
depend on deep rooting to sustain evapotranspiration during the
dry season, which may help control the length of the dry season
(see, e.g., Section 7.2.3.2). Da Rocha et al. (2004) also observed
that hydraulic lift recharged the forest upper soil pro
fi
les each
night. At Tapajós, the forest showed no signs of drought stress
allowing uniformly high carbon uptake throughout the dry
season (July through December 2000; Da Rocha et al., 2004;
Goulden et al., 2004). Tibet, another key region, continues to be
better characterised from observational studies (e.g., Gao et al.,
2004; Hong et al., 2004). With its high elevation, hence low air
densities, heating of the atmosphere by land mixes air to a much
higher altitude than elsewhere, with implications for vertical
exchange of energy. However, the daytime water vapour mixing
ratio in this region decreases rapidly with increasing altitude
(Yang et al., 2004), indicating a strong insertion of dry air from
above or by lateral transport.
7.2.3.6
Connecting Changing Vegetation to Changing
Climate
Only large-scale patterns are assessed here. Analysis of
satellite-sensed vegetation greenness and meteorological station
data suggest an enhanced plant growth and lengthened growing
season duration at northern high latitudes since the 1980s (Zhou
509
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
et al., 2001, 2003c). This effect is further supported by modelling
linked to observed climate data (Lucht et al., 2002). Nemani et
al. (2002, 2003) suggest that increased rainfall and humidity
spurred plant growth in the USA and that climate changes may
have eased several critical climatic constraints to plant growth
and thus increased terrestrial net primary production.
7.2.4
Modelling the Coupling of Vegetation,
Moisture Availability, Precipitation and
Surface Temperature
7.2.4.1
How do Models of Vegetation Control Surface
Water Fluxes?
Box 7.1 provides a general description of water
fl
uxes from
surface to atmosphere. The most important factors affected
by vegetation are soil water availability, leaf area and surface
roughness. Whether water has been intercepted on the surface of
the leaves or its loss is only from the leaf interior as controlled
by stomata makes a large difference. Shorter vegetation with
more leaves has the most latent heat
fl
ux and the least sensible
fl
ux. Replacement of forests with shorter vegetation together
with the normally assumed higher albedo could then cool the
surface. However, if the replacement vegetation has much less
foliage or cannot access soil water as successfully, a warming
may occur. Thus, deforestation can modify surface temperatures
by up to several degrees celsius in either direction depending
on what type of vegetation replaces the forest and the climate
regime. Drier air can increase evapotranspiration, but leaves
may decrease their stomatal conductance to counter this effect.
7.2.4.2
Feedbacks Demonstrated Through Simple Models
In semi-arid systems, the occurrence and amounts of
precipitation can be highly variable from year to year. Are
there mechanisms whereby the growth of vegetation in times
of adequate precipitation can act to maintain the precipitation?
Various analyses with simple models have demonstrated
how this might happen (Zeng et al., 2002; Foley et al., 2003;
G. Wang, et al., 2004; X. Zeng et al., 2004). Such models
demonstrate how assumed feedbacks between precipitation and
surface
fl
uxes generated by dynamic vegetation may lead to the
possibility of transitions between multiple equilibria for two
soil moisture and precipitation regimes. That is, the extraction
of water by roots and shading of soil by plants can increase
precipitation and maintain the vegetation, but if the vegetation
is removed, it may not be able to be restored for a long period.
The Sahel region between the deserts of North Africa and the
African equatorial forests appears to most readily generate such
an alternating precipitation regime.
7.2.4.3
Consequences of Changing Moisture Availability
and Land Cover
Soil moisture control of the partitioning of energy between
sensible and latent heat
fl
ux is very important for local and
regional temperatures, and possibly their coupling to
precipitation. Oglesby et al. (2002) carried out a study
starting with dry soil where the dryness of the soil over the
US Great Plains for at least the
fi
rst several summer months
of their integration produced a warming of about 10°C to
20°C. Williamson et al. (2005), have shown that
fl
aws in
model formulation of thunderstorms can cause excessive
evapotranspiration that lowers temperatures by more than
1°C. Many modelling studies have demonstrated that changing
land cover can have local and regional climate impacts that
are comparable in magnitude to temperature and precipitation
changes observed over the last several decades as reported in
Chapter 3. However, since such regional changes can be of both
signs, the global average impact is expected to be small. Current
literature has large disparities in conclusions. For example,
Snyder et al. (2004) found that removal of northern temperate
forests gave a summer warming of 1.3°C and a reduction in
precipitation of 1.5 mm day
-1
. Conversely, Oleson et al. (2004)
found that removal of temperate forests in the USA would cool
summer temperatures by 0.4°C to 1.5°C and probably increase
precipitation, depending on the details of the model and
prescription of vegetation. The discrepancy between these two
studies may be largely an artefact of different assumptions. The
fi
rst study assumes conversion of forest to desert and the second
to crops. Such studies collectively demonstrate a potentially
important impact of human activities on climate through land
use modi
fi
cation.
Other recent such studies illustrate various aspects of this
issue. Maynard and Royer (2004) address the sensitivity
to different parameter changes in African deforestation
experiments and
fi
nd that changes in roughness, soil depth,
vegetation cover, stomatal resistance, albedo and leaf area
index all could make signi
fi
cant contributions. Voldoire and
Royer (2004)
fi
nd that such changes may affect temperature
and precipitation extremes more than means, in particular the
daytime maximum temperature and the drying and temperature
responses associated with El Niño events. Guillevic et al. (2002)
address the importance of interannual leaf area variability as
inferred from Advanced Very High Resolution Radiometer
(AVHRR) satellite data, and infer a sensitivity of climate to this
variation. In contrast, Lawrence and Slingo (2004)
fi
nd little
difference in climate simulations that use annual mean vegetation
characteristics compared with those that use a prescribed
seasonal cycle. However, they do suggest model modi
fi
cations
that would give a much larger sensitivity. Osborne et al. (2004)
examine effects of changing tropical soils and vegetation:
variations in vegetation produce variability in surface
fl
uxes
and their coupling to precipitation. Thus, interactive vegetation
can promote additional variability of surface temperature and
precipitation as analysed by Cruci
fi
x et al. (2005). Marengo
and Nobre (2001) found that removal of vegetation led to a
decrease in precipitation and evapotranspiration and a decrease
in moisture convergence in central and northern Amazonia.
Oyama and Nobre (2004) show that removal of vegetation in
northeast Brazil would substantially decrease precipitation.
510
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.2.4.4
Mechanisms for Modi
fi
cation of Precipitation by
Spatial Heterogeneity
Clark et al. (2004) show an example of a ‘squall-line’
simulation where soil moisture variation at the scale of the
rainfall modi
fi
es the rainfall pattern. Pielke (2001), Weaver et al.
(2002) and S. Roy et al. (2003) also address various aspects of
small-scale precipitation coupling to land surface heterogeneity.
If deforestation occurs in patches rather than uniformly, the
consequences for precipitation could be different. Avissar et al.
(2002) and Silva Dias et al. (2002) suggest that there may be a
small increase in precipitation (of the order of 10%) resulting
from partial deforestation as a consequence of the mesoscale
circulations triggered by the deforestation.
7.2.4.5
Interactive Vegetation Response Variables
Prognostic approaches estimate leaf cover based on
physiological processes (e.g., Arora and Boer, 2005). Levis
and Bonan (2004) discuss how spring leaf emergence in mid-
latitude forests provides a negative feedback to rapid increases
in temperature. The parametrization of water uptake by roots
contributes to the computed soil water pro
fi
le (Feddes et al., 2001;
Barlage and Zeng, 2004), and efforts are being made to make the
roots interactive (e.g., Arora and Boer, 2003). Dynamic vegetation
models have advanced and now explicitly simulate competition
between plant functional types (e.g., Bonan et al., 2003; Sitch et
al., 2003; Arora and Boer, 2006). New coupled climate-carbon
models (Betts et al., 2004; Huntingford et al., 2004) demonstrate
the possibility of large feedbacks between future climate change
and vegetation change, discussed further in Section 7.3.5 (i.e.,
a die back of Amazon vegetation and reductions in Amazon
precipitation). They also indicate that the physiological forcing of
stomatal closure by rising atmospheric CO
2
levels could contribute
20% to the rainfall reduction. Levis et al. (2004) demonstrate how
African rainfall and dynamic vegetation could change each other.
7.2.5
Evaluation of Models Through
Intercomparison
Intercomparison of vegetation models usually involves
comparing surface
fl
uxes and their feedbacks. Henderson-
Sellers et al. (2003), in comparing the surface
fl
uxes among
20 models, report over an order of magnitude range among
sensible
fl
uxes of different models. However, recently
developed models cluster more tightly. Irannejad et al. (2003)
developed a statistical methodology to
fi
t monthly
fl
uxes from
a large number of climate models to a simple linear statistical
model, depending on factors such as monthly net radiation and
surface relative humidity. Both the land and atmosphere models
are major sources of uncertainty for feedbacks. Irannejad et al.
fi
nd that coupled models agree more closely due to offsetting
differences in the atmospheric and land models. Modelling
studies have long reported that soil moisture can in
fl
uence
precipitation. Only recently, however, have there been
attempts to quantify this coupling from a statistical viewpoint
(Dirmeyer, 2001; Koster and Suarez, 2001; Koster et al., 2002;
Reale and Dirmeyer, 2002; Reale et al., 2002; Koster et al.,
2003; Koster and Suarez, 2004). Koster et al. (2004, 2006)
and Guo et al. (2006) report on a new model intercomparison
activity, the Global Land Atmosphere Coupling Experiment
(GLACE), which compares among climate models differences
in precipitation variability caused by interaction with soil
moisture. Using an experimental protocol to generate ensembles
of simulations with soil moisture that is either prescribed or
interactive as it evolves in time, they report a wide range of
differences between models (Figure 7.2). Lawrence and Slingo
(2005) show that the relatively weak coupling strength of the
Hadley Centre model results from its atmospheric component.
There is yet little con
fi
dence in this feedback component of
climate models and therefore its possible contribution to global
warming (see Chapter 8).
Figure 7.2.
Coupling strength (a nondimensional pattern similarity diagnostic defi ned in Koster et al., 2006) between summer rainfall and soil water in models assessed by
the GLACE study (Guo et al., 2006), divided into how strongly soil water causes evaporation (including from plants) and how strongly this evaporation causes rainfall. The soil
water-precipitation coupling is scaled up by a factor of 10, and the two indices for evaporation to precipitation coupling given in the study are averaged. Models include the
Geophysical Fluid Dynamics Laboratory (GFDL) model, the National Aeronautics and Space Administration (NASA) Seasonal to Interannual Prediction Program (NSIPP) model,
the National Center for Atmospheric Research Community Atmosphere Model (CAM3), the Canadian Centre for Climate Modelling and Analysis (CCCma) model, the Centre for
Climate System Research (CCSR) model, the Bureau of Meteorology Research Centre (BMRC) model and the Hadley Centre Atmospheric Model version 3 (HadAM3).
511
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.2.6
Linking Biophysical to Biogeochemical and
Ecohydrological Components
Soil moisture and surface temperatures work together in
response to precipitation and radiative inputs. Vegetation
in
fl
uences these terms through its controls on energy and water
fl
uxes, and through these
fl
uxes, precipitation. It also affects the
radiative heating. Clouds and precipitation are affected through
modi
fi
cations of the temperature and water vapour content of
near-surface air. How the feedbacks of land to the atmosphere
work remains dif
fi
cult to quantify from either observations
or modelling (as addressed in Sections 7.2.3.2 and 7.2.5.1).
Radiation feedbacks depend on vegetation or cloud cover
that has changed because of changing surface temperatures
or moisture conditions. How such conditions may promote or
discourage the growth of vegetation is established by various
ecological studies. The question of how vegetation will change
its distribution at large scales and the consequent changes in
absorbed radiation is quanti
fi
ed through remote sensing studies.
At desert margins, radiation and precipitation feedbacks may
act jointly with vegetation. Radiation feedbacks connected to
vegetation may be most pronounced at the margins between
boreal forests and tundra and involve changes in the timing of
snowmelt. How energy is transferred from the vegetation to
underlying snow surfaces is understood in general terms but
remains problematic in modelling and process details. Dynamic
vegetation models (see Section 7.2.4.5) synthesize current
understanding.
Changing soil temperatures and snow cover affect soil
microbiota and their processing of soil organic matter. How are
nutrient supplies modi
fi
ed by these surface changes or delivery
from the atmosphere? In particular, the treatment of carbon
fl
uxes (addressed in more detail in Section 7.3) may require
comparable or more detail in the treatment of N cycling (as
attempted by S. Wang, et al., 2002; Dickinson et al., 2003).
The challenge is to establish better process understanding at
local scales and appropriately incorporate this understanding
into global models. The Coupled Carbon-Cycle Climate Model
Intercomparison Project (C
4
MIP) simulations described in
Section 7.3.5 are a
fi
rst such effort.
Biomass burning is a major mechanism for changing
vegetation cover and generation of atmospheric aerosols and is
directly coupled to the land climate variables of moisture and
near-surface winds, as addressed for the tropics by Hoffman et
al. (2002). The aerosol plume produced by biomass burning at
the end of the dry season contains black carbon that absorbs
radiation. The combination of a cooler surface due to lack of
solar radiation and a warmer boundary layer due to absorption
of solar radiation increases the thermal stability and reduces
cloud formation, and thus can reduce rainfall. Freitas et al.
(2005) indicate the possibility of rainfall decrease in the Plata
Basin as a response to the radiative effect of the aerosol load
transported from biomass burning in the Cerrado and Amazon
regions. Aerosols and clouds reduce the availability of visible
light needed by plants for photosynthesis. However, leaves in
full sun may be light saturated, that is, they do not develop
suf
fi
cient enzymes to utilise that level of light. Leaves that
are shaded, however, are generally light limited. They are
only illuminated by diffuse light scattered by overlying leaves
or by atmospheric constituents. Thus, an increase in diffuse
light at the expense of direct light may promote leaf carbon
assimilation and transpiration (Roderick et al., 2001; Cohan
et al., 2002; Gu et al., 2002, 2003). Yamasoe et al. (2006)
report the
fi
rst observational tower evidence for this effect in
the tropics. Diffuse radiation resulting from the Mt. Pinatubo
eruption may have created an enhanced terrestrial carbon sink
(Roderick et al., 2001; Gu et al., 2003). Angert et al. (2004)
provide an analysis that rejects this hypothesis relative to other
possible mechanisms.
7.3
The Carbon Cycle and the
Climate System
7.3.1
Overview of the Global Carbon Cycle
7.3.1.1
The Natural Carbon Cycle
Over millions of years, CO
2
is removed from the atmosphere
through weathering by silicate rocks and through burial in
marine sediments of carbon
fi
xed by marine plants (e.g.,
Berner, 1998). Burning fossil fuels returns carbon captured by
plants in Earth’s geological history to the atmosphere. New ice
core records show that the Earth system has not experienced
current atmospheric concentrations of CO
2
, or indeed of CH
4
,
for at least 650 kyr – six glacial-interglacial cycles. During that
period the atmospheric CO
2
concentration remained between
180 ppm (glacial maxima) and 300 ppm (warm interglacial
periods) (Siegenthaler et al., 2005). It is generally accepted that
during glacial maxima, the CO
2
removed from the atmosphere
was stored in the ocean. Several causal mechanisms have been
identi
fi
ed that connect astronomical changes, climate, CO
2
and
other greenhouse gases, ocean circulation and temperature,
biological productivity and nutrient supply, and interaction with
ocean sediments (see Box 6.2).
Prior to 1750, the atmospheric concentration of CO
2
had
been relatively stable between 260 and 280 ppm for 10 kyr
(Box 6.2). Perturbations of the carbon cycle from human
activities were insigni
fi
cant relative to natural variability.
Since 1750, the concentration of CO
2
in the atmosphere has
risen, at an increasing rate, from around 280 ppm to nearly
380 ppm in 2005 (see Figure 2.3 and FAQ 2.1, Figure 1). The
increase in atmospheric CO
2
concentration results from human
activities: primarily burning of fossil fuels and deforestation,
but also cement production and other changes in land use and
management such as biomass burning, crop production and
conversion of grasslands to croplands (see FAQ 7.1). While
human activities contribute to climate change in many direct
and indirect ways, CO
2
emissions from human activities are
considered the single largest anthropogenic factor contributing
to climate change (see FAQ 2.1, Figure 2). Atmospheric CH
4
512
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Frequently Asked Question 7.1
Are the Increases in Atmospheric Carbon Dioxide
and Other Greenhouse Gases During the Industrial Era
Caused by Human Activities?
Yes, the increases in atmospheric carbon dioxide (CO
2
) and
other greenhouse gases during the industrial era are caused by hu-
man activities. In fact, the observed increase in atmospheric CO
2
concentrations does not reveal the full extent of human emissions in
that it accounts for only 55% of the CO
2
released by human activity
since 1959. The rest has been taken up by plants on land and by
the oceans. In all cases, atmospheric concentrations of greenhouse
gases, and their increases, are determined by the balance between
sources (emissions of the gas from human activities and natural
systems) and sinks (the removal of the gas from the atmosphere
by conversion to a different chemical compound). Fossil fuel com-
bustion (plus a smaller contribution from cement manufacture) is
responsible for more than 75% of human-caused CO
2
emissions.
Land use change (primarily deforestation) is responsible for the re-
mainder. For methane, another important greenhouse gas, emis-
sions generated by human activities exceeded natural emissions
over the last 25 years. For nitrous oxide, emissions generated by
human activities are equal to natural emissions to the atmosphere.
Most of the long-lived halogen-containing gases (such as chloro-
fl uorcarbons) are manufactured by humans, and were not present in
the atmosphere before the industrial era. On average, present-day
tropospheric ozone has increased 38% since pre-industrial times,
and the increase results from atmospheric reactions of short-lived
pollutants emitted by human activity. The concentration of CO
2
is now 379 parts per million (ppm) and methane is greater than
1,774 parts per billion (ppb), both very likely much higher than
any time in at least 650 kyr (during which CO
2
remained between
180 and 300 ppm and methane between 320 and 790 ppb). The
recent rate of change is dramatic and unprecedented; increases in
CO
2
never exceeded 30 ppm in 1 kyr – yet now CO
2
has risen by 30
ppm in just the last 17 years.
Carbon Dioxide
Emissions of CO
2
(Figure 1a) from fossil fuel combustion,
with contributions from cement manufacture, are responsible
for more than 75% of the increase in atmospheric CO
2
concen-
tration since pre-industrial times. The remainder of the increase
comes from land use changes dominated by deforestation (and
associated biomass burning) with contributions from changing
agricultural practices. All these increases are caused by human
activity. The natural carbon cycle cannot explain the observed
atmospheric increase of 3.2 to 4.1 GtC yr
–1
in the form of CO
2
over the last 25 years. (One GtC equals 10
15
grams of carbon,
i.e., one billion tonnes.)
Natural processes such as photosynthesis, respiration, decay
and sea surface gas exchange lead to massive exchanges, sources
and sinks of CO
2
between the land and atmosphere (estimated at
~120 GtC yr
–1
) and the ocean and atmosphere (estimated at ~90
GtC yr
–1
; see figure 7.3). The natural sinks of carbon produce
a small net uptake of CO
2
of approximately 3.3 GtC yr
–1
over
the last 15 years, partially offsetting the human-caused emis-
sions. Were it not for the natural sinks taking up nearly half the
human-produced CO
2
over the past 15 years, atmospheric con-
centrations would have grown even more dramatically.
The increase in atmospheric CO
2
concentration is known to
be caused by human activities because the character of CO
2
in
the atmosphere, in particular the ratio of its heavy to light car-
bon atoms, has changed in a way that can be attributed to ad-
dition of fossil fuel carbon. In addition, the ratio of oxygen to
nitrogen in the atmosphere has declined as CO
2
has increased;
this is as expected because oxygen is depleted when fossil fuels
are burned. A heavy form of carbon, the carbon-13 isotope, is
less abundant in vegetation and in fossil fuels that were formed
from past vegetation, and is more abundant in carbon in the
oceans and in volcanic or geothermal emissions. The relative
amount of the carbon-13 isotope in the atmosphere has been
declining, showing that the added carbon comes from fossil fu-
els and vegetation. Carbon also has a rare radioactive isotope,
carbon-14, which is present in atmospheric CO
2
but absent in
fossil fuels. Prior to atmospheric testing of nuclear weapons,
decreases in the relative amount of carbon-14 showed that fos-
sil fuel carbon was being added to the atmosphere.
Halogen-Containing Gases
Human activities are responsible for the bulk of long-lived at-
mospheric halogen-containing gas concentrations. Before indus-
trialisation, there were only a few naturally occurring halogen-
containing gases, for example, methyl bromide and methyl
chloride. The development of new techniques for chemical syn-
thesis resulted in a proliferation of chemically manufactured
halogen-containing gases during the last 50 years of the 20th
century. Emissions of key halogen-containing gases produced
by humans are shown in Figure 1b. Atmospheric lifetimes range
from 45 to 100 years for the chlorofluorocarbons (CFCs) plot-
ted here, from 1 to 18 years for the hydrochlorofluorocarbons
(HCFCs), and from 1 to 270 years for the hydrofluorocarbons
(HFCs). The perfluorocarbons (PFCs, not plotted) persist in the
atmosphere for thousands of years. Concentrations of several
important halogen-containing gases, including CFCs, are now
stabilising or decreasing at the Earth’s surface as a result of the
Montreal Protocol on Substances that Deplete the Ozone Layer
and its Amendments. Concentrations of HCFCs, production of
which is to be phased out by 2030, and of the Kyoto Protocol
gases HFCs and PFCs, are currently increasing.
(continued)
513
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Tropospheric ozone concentrations are significantly higher in
urban air, downwind of urban areas and in regions of biomass
burning. The increase of 38% (20–50%) in tropospheric ozone
since the pre-industrial era (Figure 1e) is human-caused.
It is very likely that the increase in the combined radiative
forcing from CO
2
, CH
4
and N
2
O was at least six times faster be-
tween 1960 and 1999 than over any 40-year period during the
two millennia prior to the year 1800.
Methane
Methane (CH
4
) sources to the
atmosphere generated by human
activities exceed CH
4
sources from
natural systems (Figure 1c). Between
1960 and 1999, CH
4
concentrations
grew an average of at least six times
faster than over any 40-year period
of the two millennia before 1800,
despite a near-zero growth rate since
1980. The main natural source of
CH
4
to the atmosphere is wetlands.
Additional natural sources include
termites, oceans, vegetation and CH
4
hydrates. The human activities that
produce CH
4
include energy pro-
duction from coal and natural gas,
waste disposal in landfi lls, raising
ruminant animals (e.g., cattle and
sheep), rice agriculture and biomass
burning. Once emitted, CH
4
remains
in the atmosphere for approximately
8.4 years before removal, mainly
by chemical oxidation in the tropo-
sphere. Minor sinks for CH
4
include
uptake by soils and eventual destruc-
tion in the stratosphere.
Nitrous Oxide
Nitrous oxide (N
2
O) sources to the atmosphere from human
activities are approximately equal to N
2
O sources from natural
systems (Figure 1d). Between 1960 and 1999, N
2
O concentra-
tions grew an average of at least two times faster than over
any 40-year period of the two millennia before 1800. Natural
sources of N
2
O include oceans, chemical oxidation of ammonia
in the atmosphere, and soils. Tropical soils are a particularly
important source of N
2
O to the atmosphere. Human activities
that emit N
2
O include transformation of fertilizer nitrogen into
N
2
O and its subsequent emission from agricultural soils, bio-
mass burning, raising cattle and some industrial activities, in-
cluding nylon manufacture. Once emitted, N
2
O remains in the
atmosphere for approximately 114 years before removal, mainly
by destruction in the stratosphere.
Tropospheric Ozone
Tropospheric ozone is produced by photochemical reac-
tions in the atmosphere involving forerunner chemicals such as
carbon monoxide, CH
4
, volatile organic compounds and nitro-
gen oxides. These chemicals are emitted by natural biological
processes and by human activities including land use change
and fuel combustion. Because tropospheric ozone is relatively
short-lived, lasting for a few days to weeks in the atmosphere,
its distributions are highly variable and tied to the abundance
of its forerunner compounds, water vapour and sunlight.
FAQ 7.1, Figure 1.
Breakdown of contributions to the
changes in atmospheric greenhouse gas concentrations,
based on information detailed in Chapters 4 and 7. In (a)
through (d), human-caused sources are shown in orange,
while natural sources and sinks are shown in teal. In (e), hu-
man-caused tropospheric ozone amounts are in orange while
natural ozone amounts are in green. (a) Sources and sinks
of CO
2
(GtC). Each year CO
2
is released to the atmosphere
from human activities including fossil fuel combustion and
land use change. Only 57 to 60% of the CO
2
emitted from
human activity remains in the atmosphere. Some is dissolved
into the oceans and some is incorporated into plants as they
grow. Land-related fl uxes are for the 1990s; fossil fuel and cement fl uxes and net
ocean uptake are for the period 2000 to 2005. All values and uncertainty ranges are
from Table 7.1. (b) Global emissions of CFCs and other halogen-containing compounds
for 1990 (light orange) and 2002 (dark orange). These chemicals are exclusively
human-produced. Here, ‘HCFCs’ comprise HCFC-22, -141b and -142b, while ‘HFCs’
comprise HFC-23, -125, -134a and -152a. One Gg = 10
9
g (1,000 tonnes). Most data
are from reports listed in Chapter 2. (c) Sources and sinks of CH
4
for the period 1983
to 2004. Human-caused sources of CH
4
include energy production, landfi lls, ruminant
animals (e.g., cattle and sheep), rice agriculture and biomass burning. One Tg = 10
12
g (1 million tonnes). Values and uncertainties are the means and standard deviations
for CH
4
of the corresponding aggregate values from Table 7.6. (d) Sources and sinks
of N
2
O. Human-caused sources of N
2
O include the transformation of fertilizer nitrogen
into N
2
O and its subsequent emission from agricultural soils, biomass burning,
cattle and some industrial activities including nylon manufacture. Source values and
uncertainties are the midpoints and range limits from Table 7.7. N
2
O losses are from
Chapter 7.4. (e) Tropospheric ozone in the 19th and early 20th centuries and the 1990
to 2000 period. The increase in tropospheric ozone formation is human-induced, re-
sulting from atmospheric chemical reactions of pollutants emitted by burning of fossil
fuels or biofuels. The pre-industrial value and uncertainty range are from Table 4.9 of
the IPCC Third Assessment Report (TAR), estimated from reconstructed observations.
The present-day total and its uncertainty range are the average and standard devia-
tion of model results quoted in Table 7.9 of this report, excluding those from the TAR.
514
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
concentrations have similarly experienced a rapid rise from
about 700 ppb in 1750 (Flückiger et al., 2002) to about 1,775
ppb in 2005 (see Section 2.3.2): sources include fossil fuels,
land
fi
lls and waste treatment, peatlands/wetlands, ruminant
animals and rice paddies. The increase in CH
4
radiative forcing
is slightly less than one-third that of CO
2
, making it the second
most important greenhouse gas (see Chapter 2). The CH
4
cycle
is presented in Section 7.4.1.
Both CO
2
and CH
4
play roles in the natural cycle of
carbon, involving continuous
fl
ows of large amounts of
carbon among the ocean, the terrestrial biosphere and the
atmosphere, that maintained stable atmospheric concentrations
of these gases for 10 kyr prior to 1750. Carbon is converted
to plant biomass by photosynthesis. Terrestrial plants capture
CO
2
from the atmosphere; plant, soil and animal respiration
(including decomposition of dead biomass) returns carbon to
the atmosphere as CO
2
, or as CH
4
under anaerobic conditions.
Vegetation
fi
res can be a signi
fi
cant source of CO
2
and CH
4
to
the atmosphere on annual time scales, but much of the CO
2
is
recaptured by the terrestrial biosphere on decadal time scales if
the vegetation regrows.
Carbon dioxide is continuously exchanged between the
atmosphere and the ocean. Carbon dioxide entering the surface
ocean immediately reacts with water to form bicarbonate
(HCO
3
–
) and carbonate (CO
3
2–
) ions. Carbon dioxide, HCO
3
–
and CO
3
2–
are collectively known as dissolved inorganic carbon
(DIC). The residence time of CO
2
(as DIC) in the surface ocean,
relative to exchange with the atmosphere and physical exchange
with the intermediate layers of the ocean below, is less than
a decade. In winter, cold waters at high latitudes, heavy and
enriched with CO
2
(as DIC) because of their high solubility,
sink from the surface layer to the depths of the ocean. This
localised sinking, associated with the Meridional Overturning
Circulation (MOC; Box 5.1) is termed the ‘solubility pump’.
Over time, it is roughly balanced by a distributed diffuse upward
transport of DIC primarily into warm surface waters.
Phytoplankton take up carbon through photosynthesis.
Some of that sinks from the surface layer as dead organisms
and particles (the ‘biological pump’), or is transformed into
dissolved organic carbon (DOC). Most of the carbon in sinking
particles is respired (through the action of bacteria) in the
surface and intermediate layers and is eventually recirculated
to the surface as DIC. The remaining particle
fl
ux reaches
abyssal depths and a small fraction reaches the deep ocean
sediments, some of which is re-suspended and some of which
is buried. Intermediate waters mix on a time scale of decades
to centuries, while deep waters mix on millennial time scales.
Several mixing times are required to bring the full buffering
capacity of the ocean into effect (see Section 5.4 for long-term
observations of the ocean carbon cycle and their consistency
with ocean physics).
Together the solubility and biological pumps maintain a
vertical gradient in CO
2
(as DIC) between the surface ocean
(low) and the deeper ocean layers (high), and hence regulate
exchange of CO
2
between the atmosphere and the ocean. The
strength of the solubility pump depends globally on the strength
of the MOC, surface ocean temperature, salinity, strati
fi
cation
and ice cover. The ef
fi
ciency of the biological pump depends
on the fraction of photosynthesis exported from the surface
ocean as sinking particles, which can be affected by changes
in ocean circulation, nutrient supply and plankton community
composition and physiology.
In Figure 7.3 the natural or unperturbed exchanges (estimated
to be those prior to 1750) among oceans, atmosphere and land are
shown by the black arrows. The gross natural
fl
uxes between the
terrestrial biosphere and the atmosphere and between the oceans
and the atmosphere are (circa 1995) about 120 and 90 GtC yr
–1
,
respectively. Just under 1 GtC yr
–1
of carbon is transported from
the land to the oceans via rivers either dissolved or as suspended
particles (e.g., Richey, 2004). While these
fl
uxes vary from year
to year, they are approximately in balance when averaged over
longer time periods. Additional small natural
fl
uxes that are
important on longer geological time scales include conversion
of labile organic matter from terrestrial plants into inert organic
carbon in soils, rock weathering and sediment accumulation
(‘reverse weathering’), and release from volcanic activity. The
net
fl
uxes in the 10 kyr prior to 1750, when averaged over
decades or longer, are assumed to have been less than about
0.1 GtC yr
–1
. For more background on the carbon cycle, see
Prentice et al. (2001), Field and Raupach (2004) and Sarmiento
and Gruber (2006).
7.3.1.2
Perturbations of the Natural Carbon Cycle from
Human Activities
The additional burden of CO
2
added to the atmosphere by
human activities, often referred to as ‘anthropogenic CO
2
’ leads
to the current ‘perturbed’ global carbon cycle. Figure 7.3 shows
that these ‘anthropogenic emissions’ consist of two fractions:
(i) CO
2
from fossil fuel burning and cement production, newly
released from hundreds of millions of years of geological storage
(see Section 2.3) and (ii) CO
2
from deforestation and agricultural
development, which has been stored for decades to centuries.
Mass balance estimates and studies with other gases indicate
that the net land-atmosphere and ocean-atmosphere
fl
uxes have
become signi
fi
cantly different from zero, as indicated by the
red arrows in Figure 7.3 (see also Section 7.3.2). Although the
anthropogenic
fl
uxes of CO
2
between the atmosphere and both
the land and ocean are just a few percent of the gross natural
fl
uxes, they have resulted in measurable changes in the carbon
content of the reservoirs since pre-industrial times as shown
in red. These perturbations to the natural carbon cycle are the
dominant driver of climate change because of their persistent
effect on the atmosphere. Consistent with the response function
to a CO
2
pulse from the Bern Carbon Cycle Model (see footnote
(a) of Table 2.14), about 50% of an increase in atmospheric CO
2
will be removed within 30 years, a further 30% will be removed
within a few centuries and the remaining 20% may remain in
the atmosphere for many thousands of years (Prentice et al.,
2001; Archer, 2005; see also Sections 7.3.4.2 and 10.4)
About 80% of anthropogenic CO
2
emissions during the 1990s
resulted from fossil fuel burning, with about 20% from land use
515
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
change (primarily deforestation) (Table 7.1). Almost 45% of
combined anthropogenic CO
2
emissions (fossil fuel plus land
use) have remained in the atmosphere. Oceans are estimated to
have taken up approximately 30% (about 118 ± 19 GtC: Sabine
et al., 2004a; Figure 7.3), an amount that can be accounted for
by increased atmospheric concentration of CO
2
without any
change in ocean circulation or biology. Terrestrial ecosystems
have taken up the rest through growth of replacement vegetation
on cleared land, land management practices and the fertilizing
effects of elevated CO
2
and N deposition (see Section 7.3.3).
Because CO
2
does not limit photosynthesis signi
fi
cantly
in the ocean, the biological pump does not take up and store
anthropogenic carbon directly. Rather, marine biological cycling
of carbon may undergo changes due to high CO
2
concentrations,
via feedbacks in response to a changing climate. The speed with
which anthropogenic CO
2
is taken up effectively by the ocean,
however, depends on how quickly surface waters are transported
and mixed into the intermediate and deep layers of the ocean. A
considerable amount of anthropogenic CO
2
can be buffered or
neutralized by dissolution of CaCO
3
from surface sediments in
the deep sea, but this process requires many thousands of years.
The increase in the atmospheric CO
2
concentration relative
to the emissions from fossil fuels and cement production only
is de
fi
ned here as the ‘airborne fraction’.
2
Land emissions,
although signi
fi
cant, are not included in this de
fi
nition due
to the dif
fi
culty of quantifying their contribution, and to the
complication that much land emission from logging and
clearing of forests may be compensated a few years later by
uptake associated with regrowth. The ‘airborne fraction of total
emissions’ is thus de
fi
ned as the atmospheric CO
2
increase as a
fraction of total anthropogenic CO
2
emissions, including the net
land use
fl
uxes. The airborne fraction varies from year to year
mainly due to the effect of interannual variability in land uptake
(see Section 7.3.2).
7.3.1.3
New Developments in Knowledge of the Carbon
Cycle Since the Third Assessment Report
Sections 7.3.2 to 7.3.5 describe where knowledge and
understanding have advanced signi
fi
cantly since the Third
Assessment Report (TAR). In particular, the budget of
anthropogenic CO
2
(shown by the red
fl
uxes in Figure 7.3)
can be calculated with improved accuracy. In the ocean, newly
available high-quality data on the ocean carbon system have
been used to construct robust estimates of the cumulative
ocean burden of anthropogenic carbon (Sabine et al., 2004a)
and associated changes in the carbonate system (Feely et al.,
2004). The pH in the surface ocean is decreasing, indicating the
need to understand both its interaction with a changing climate
and the potential impact on organisms in the ocean (e.g., Orr
et al., 2005; Royal Society, 2005). On land, there is a better
understanding of the contribution to the buildup of CO
2
in the
atmosphere since 1750 associated with land use and of how
the land surface and the terrestrial biosphere interact with a
changing climate. Globally, inverse techniques used to infer the
magnitude and location of major
fl
uxes in the global carbon
Figure 7.3.
The global carbon cycle for the 1990s, showing the main annual fl uxes in GtC yr
–1
: pre-industrial ‘natural’ fl uxes in black and ‘anthropogenic’ fl uxes in red (modi-
fi ed from Sarmiento and Gruber, 2006, with changes in pool sizes from Sabine et al., 2004a). The net terrestrial loss of –39 GtC is inferred from cumulative fossil fuel emissions
minus atmospheric increase minus ocean storage. The loss of –140 GtC from the ‘vegetation, soil and detritus’ compartment represents the cumulative emissions from land use
change (Houghton, 2003), and requires a terrestrial biosphere sink of 101 GtC (in Sabine et al., given only as ranges of –140 to –80 GtC and 61 to 141 GtC, respectively; other
uncertainties given in their Table 1). Net anthropogenic exchanges with the atmosphere are from Column 5 ‘AR4’ in Table 7.1. Gross fl uxes generally have uncertainties of more
than ±20% but fractional amounts have been retained to achieve overall balance when including estimates in fractions of GtC yr
–1
for riverine transport, weathering, deep ocean
burial, etc. ‘GPP’ is annual gross (terrestrial) primary production. Atmospheric carbon content and all cumulative fl uxes since 1750 are as of end 1994.
2
This defi nition follows the usage of C. Keeling, distinct from that of Oeschger et al. (1980).
516
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
1980s
1990s
2000–2005c
TAR
TAR
revised
a
TAR
AR4
AR4
Atmospheric Increase
b
3.3 ± 0.1
3.3 ± 0.1
3.2 ± 0.1
3.2 ± 0.1
4.1 ± 0.1
Emissions (fossil + cement)
c
5.4 ± 0.3
5.4 ± 0.3
6.4 ± 0.4
6.4 ± 0.4
7.2 ± 0.3
Net ocean-to-atmosphere fl ux
d
–1.9 ± 0.6
–1.8 ± 0.8
–1.7 ± 0.5
–2.2 ± 0.4
–2.2 ± 0.5
Net land-to-atmosphere fl ux
e
–0.2 ± 0.7
–0.3 ± 0.9
–1.4 ± 0.7
–1.0 ± 0.6
–0.9 ± 0.6
Partitioned as follows
Land use change fl ux
1.7
(0.6 to 2.5)
1.4
(0.4 to 2.3)
n.a.
1.6
(0.5 to 2.7)
n.a.
Residual terrestrial sink
–1.9
(–3.8 to –0.3)
–1.7
(–3.4 to 0.2)
n.a.
–2.6
(–4.3 to –0.9)
n.a.
Table 7.1.
The global carbon budget (GtC yr
–1
); errors represent ±1 standard deviation uncertainty estimates and not interannual variability, which is larger. The atmospheric
increase (fi rst line) results from fl uxes to and from the atmosphere: positive fl uxes are inputs to the atmosphere (emissions); negative fl uxes are losses from the atmosphere
(sinks); and numbers in parentheses are ranges. Note that the total sink of anthropogenic CO
2
is well constrained. Thus, the ocean-to-atmosphere and land-to-atmosphere
fl uxes are negatively correlated: if one is larger, the other must be smaller to match the total sink, and vice versa.
Notes:
a
TAR values revised according to an ocean heat content correction for ocean oxygen fl uxes (Bopp et al., 2002) and using the Fourth Assessment Report (AR4) best
estimate for the land use change fl ux given in Table 7.2.
b
Determined from atmospheric CO
2
measurements (Keeling and Whorf, 2005, updated by S. Piper until 2006) at Mauna Loa (19°N) and South Pole (90°S) stations,
consistent with the data shown in Figure 7.4, using a conversion factor of 2.12 GtC yr
–1
= 1 ppm.
c
Fossil fuel and cement emission data are available only until 2003 (Marland et al., 2006). Mean emissions for 2004 and 2005 were extrapolated from energy use data
with a trend of 0.2 GtC yr
–1
.
d
For the 1980s, the ocean-to-atmosphere and land-to-atmosphere fl uxes were estimated using atmospheric O
2
:N
2
and CO
2
trends, as in the TAR. For the 1990s, the
ocean-to-atmosphere fl ux alone is estimated using ocean observations and model results (see Section 7.3.2.2.1), giving results identical to the atmospheric O
2
:N
2
method (Manning and Keeling, 2006), but with less uncertainty. The net land-to-atmosphere fl ux then is obtained by subtracting the ocean-to-atmosphere fl ux from
the total sink (and its errors estimated by propagation). For 2000 to 2005, the change in ocean-to-atmosphere fl ux was modelled (Le Quéré et al., 2005) and added
to the mean ocean-to-atmosphere fl ux of the 1990s. The error was estimated based on the quadratic sum of the error of the mean ocean fl ux during the 1990s and
the root mean square of the fi ve-year variability from three inversions and one ocean model presented in Le Quéré et al. (2003).
e
Balance of emissions due to land use change and a residual land sink. These two terms cannot be separated based on current observations.
Figure 7.4.
Changes in global atmospheric CO
2
concentrations. (a) Annual (bars) and fi ve-year mean (lower black line) changes in global CO
2
concentrations, from Scripps
Institution of Oceanography observations (mean of South Pole and Mauna Loa; Keeling and Whorf, 2005, updated). The upper stepped line shows annual increases that would
occur if 100% of fossil fuel emissions (Marland et al., 2006, updated as described in Chapter 2) remained in the atmosphere, and the red line shows fi ve-year mean annual
increases from National Oceanic and Atmospheric Administration (NOAA) data (mean of Samoa and Mauna Loa; Tans and Conway, 2005, updated). (b) Fraction of fossil fuel
emissions remaining in the atmosphere (‘airborne fraction’) each year (bars), and fi ve-year means (solid black line) (Scripps data) (mean since 1958 is 0.55). Note the anoma-
lously low airborne fraction in the early 1990s.
517
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
cycle have continued to mature, re
fl
ecting both re
fi
nement
of the techniques and the availability of new observations.
During preparation of the TAR, inclusion of the carbon cycle
in climate models was new. Now, results from the
fi
rst C
4
MIP
are available: when the carbon cycle is included, the models
consistently simulate climate feedbacks to land and ocean
carbon cycles that tend to reduce uptake of CO
2
by land and
ocean from 1850 to 2100 (see Section 7.3.5).
7.3.2
The Contemporary Carbon Budget
7.3.2.1 Atmospheric
Increase
The atmospheric CO
2
increase is measured with great
accuracy at various monitoring stations (see Chapter 2; and
Keeling and Whorf, 2005 updated by S. Piper through 2006).
The mean yearly increase in atmospheric CO
2
(the CO
2
‘growth
rate’) is reported in Table 7.1. Atmospheric CO
2
has continued
to increase since the TAR (Figure 7.4), and the rate of increase
appears to be higher, with the average annual increment rising
from 3.2 ± 0.1 GtC yr
–1
in the 1990s to 4.1 ± 0.1 GtC yr
–1
in
the period 2000 to 2005. The annual increase represents the net
effect of several processes that regulate global land-atmosphere
and ocean-atmosphere
fl
uxes, examined below. The ‘airborne
fraction’ (atmospheric increase in CO
2
concentration/fossil fuel
emissions) provides a basic benchmark for assessing short- and
long-term changes in these processes. From 1959 to the present,
the airborne fraction has averaged 0.55, with remarkably little
variation when block-averaged into
fi
ve-year bins (Figure 7.4).
Thus, the terrestrial biosphere and the oceans together have
consistently removed 45% of fossil CO
2
for the last 45 years,
and the recent higher rate of atmospheric CO
2
increase largely
re
fl
ects increased fossil fuel emissions. Year-to-year
fl
uctuations
in the airborne fraction are associated with major climatic
events (see Section 7.3.2.4). The annual increase in 1998, 2.5
ppm, was the highest ever observed, but the airborne fraction
(0.82) was no higher than values observed several times in prior
decades. The airborne fraction dropped signi
fi
cantly below the
average in the early 1990s, and preliminary data suggest it may
have risen above the average in 2000 to 2005.
The inter-hemispheric gradient of CO
2
provides additional
evidence that the increase in atmospheric CO
2
is caused
primarily by NH sources. The excess atmospheric CO
2
in the
NH compared with the Southern Hemisphere (SH),
Δ
CO
2
N-S
,
has increased in proportion to fossil fuel emission rates (which
are predominantly in the NH) at about 0.5 ppm per (GtC yr
–1
)
(Figure 7.5). The intercept of the best-
fi
t line indicates that,
without anthropogenic emissions, atmospheric CO
2
would be
0.8 ppm higher in the SH than in the NH, presumably due to
transport of CO
2
by the ocean circulation. The consistency
of the airborne fraction and the relationship between
Δ
CO
2
N-S
and fossil fuel emissions suggest broad consistency
in the functioning of the carbon cycle over the period. There
are interannual
fl
uctuations in
Δ
CO
2
N-S
as large as ±0.4 ppm, at
least some of which may be attributed to changes in atmospheric
circulation (Dargaville et al., 2000), while others may be due to
shifts in sources and sinks, such as large forest
fi
res.
7.3.2.1.1
Fossil fuel and cement emissions
Fossil fuel and cement emissions rose from 5.4 ± 0.3
GtC yr
–1
in the 1980s to 6.4 ± 0.4 GtC yr
–1
in the 1990s
(Marland et al., 2006). They have continued to increase between
the 1990s and 2000 to 2005, climbing to 7.2 ± 0.3 GtC yr
–1
.
These numbers are estimated based upon international energy
statistics for the 1980 to 2003 period (Marland et al., 2006) with
extrapolated trends for 2004 to 2005 (see Table 7.1). The error
(±1
standard deviation) for fossil fuel and cement emissions
is of the order of 5% globally. Cement emissions are small
compared with fossil fuel emissions (roughly 3% of the total).
7.3.2.1.2
Land use change
During the past two decades, the CO
2
fl
ux caused by land
use changes has been dominated by tropical deforestation.
Agriculture and exploitation of forest resources have reached
into formerly remote areas of old growth forest in the tropics,
in contrast to mid-latitudes where exploitation previously
eliminated most old growth forests. The land use change
fl
uxes
reported in this section include explicitly some accumulation of
carbon by regrowing vegetation (e.g., Houghton et al., 2000).
In the TAR, the global land use
fl
ux, adapted from Houghton
(1999), was estimated to be 1.7 (0.6–2.5) GtC yr
–1
for the
1980s. No estimate was available at the time for the 1990s. This
estimate is based on a ‘bookkeeping’ carbon model prescribed
with deforestation statistics (Houghton, 1999). A markedly
lower estimate of the land use
fl
ux in the 1980s (Table 7.2) was
obtained by McGuire et al. (2001) from four process-driven
Figure 7.5.
The difference between CO
2
concentration in the NH and SH (y axis),
computed as the difference between annual mean concentrations (ppm) at Mauna
Loa and the South Pole (Keeling and Whorf, 2005, updated), compared with annual
fossil fuel emissions (x axis; GtC; Marland, et al., 2006), with a line showing the best
fi t. The observations show that the north-south difference in CO
2
increases propor-
tionally with fossil fuel use, verifying the global impact of human-caused emissions.
518
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
terrestrial carbon models, prescribed with changes in cropland
area from Ramankutty and Foley (1999). The higher land use
emissions of Houghton (2003a) may re
fl
ect both the additional
inclusion of conversion of forest to pasture and the use of a
larger cropland expansion rate than the one of Ramankutty and
Foley (1999), as noted by Jain and Yang (2005). Houghton
(2003a) updated the land use
fl
ux to 2.0 ± 0.8 GtC yr
–1
for the
1980s and 2.2 ± 0.8 GtC yr
–1
for the 1990s (see Table 7.2). This
update gives higher carbon losses from tropical deforestation
than those in the TAR (Houghton 2003b).
In addition, DeFries et al. (2002) estimated a tropical
land use
fl
ux of 0.7 (0.4–1.0) GtC yr
–1
for the 1980s and 1.0
(0.5–1.6) GtC yr
–1
for the 1990s, using the same bookkeeping
approach as Houghton (1999) but driven by remotely sensed
data on deforested areas. A similar estimate was independently
produced by Achard et al. (2004) for the 1990s, also based on
remote sensing. These different land use emissions estimates
are reported in Table 7.2. Although the two recent satellite-
based estimates point to a smaller source than that of Houghton
(2003a), it is premature to say that Houghton’s numbers are
overestimated. The land use carbon source has the largest
uncertainties in the global carbon budget. If a high value for the
land use source is adopted in the global budget, then the residual
land uptake over undisturbed ecosystems should be a large sink,
and vice versa. For evaluating the global carbon budget, the
mean of DeFries et al. (2002) and Houghton (2003a), which
both cover the 1980s and the 1990s (Table 7.2), was chosen and
the full range of uncertainty is reported. The fraction of carbon
emitted by fossil fuel burning, cement production and land use
changes that does not accumulate in the atmosphere must be
taken up by land ecosystems and by the oceans.
Table 7.2.
Land to atmosphere emissions resulting from land use changes during the 1990s and the 1980s (GtC yr
–1
). The Fourth Assessment Report (AR4) estimates used
in the global carbon budget (Table 7.1) are shown in bold. Positive values indicate carbon losses from land ecosystems. Uncertainties are reported as ±1 standard deviation.
Numbers in parentheses are ranges of uncertainty.
Tropical
Americas
Tropical
Africa
Tropical
Asia
Pan-Tropical
Non-tropics
Total Globe
1990s
Houghton (2003a)
a
0.8 ± 0.3
0.4 ± 0.2
1.1 ± 0.5
2.2 ± 0.6
–0.02 ± 0.5
2.2 ± 0.8
DeFries et al.
(2002)
b
0.5
(0.2 to 0.7)
0.1
(0.1 to 0.2)
0.4
(0.2 to 0.6)
1.0
(0.5 to 1.6)
n.a.
n.a.
Achard et al.
(2004)
c
0.3
(0.3 to 0.4)
0.2
(0.1 to 0.2)
0.4
(0.3 to 0.5)
0.9
(0.5 to 1.4)
n.a.
n.a.
AR4
d
0.7
(0.4 to 0.9)
0.3
(0.2 to 0.4)
0.8
(0.4 to 1.1)
1.6
(1.0 to 2.2)
–0.02
(–0.5 to +0.5)
1.6
(0.5 to 2.7)
1980s
Houghton (2003a)
a
0.8 ± 0.3
0.3 ± 0.2
0.9 ± 0.5
1.9 ± 0.6
0.06 ± 0.5
2.0 ± 0.8
DeFries et al.
(2002)
b
0.4
(0.2 to 0.5)
0.1
(0.08 to 0.14)
0.2
(0.1 to 0.3)
0.7
(0.4 to 1.0)
n.a.
n.a.
McGuire et al.
(2001)
e
0.6 to 1.2
–0.1 to +0.4
(0.6 to 1.0)
Jain and Yang
(2005)
f
0.22 to 0.24
0.08 to 0.48
0.58 to 0.34
-
-
1.33 to 2.06
TAR
g
1.7
(0.6 to 2.5)
AR4
d
0.6
(0.3 to 0.8)
0.2
(0.1 to 0.3)
0.6
(0.3 to 0.9)
1.3
(0.9 to 1.8)
0.06
(–0.4 to +0.6)
1.4
(0.4 to 2.3)
Notes:
a
His Table 2.
b
Their Table 3.
c
Their Table 2 for mean estimates with the range indicated in parentheses corresponding to their reported minimum and maximum estimates.
d
Best estimate calculated from the mean of Houghton (2003a) and DeFries et al. (2002), the only two studies covering both the 1980s and the 1990s. For non-tropical
regions where DeFries et al. have no estimate, Houghton has been used.
e
Their Table 5; range is obtained from four terrestrial carbon models.
f
The range indicated in parentheses corresponds to two simulations using the same model, but forced with different land cover change datasets from Houghton
(2003a) and DeFries et al. (2002).
g
In the TAR estimate, no values were available for the 1990s.
519
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.3.2.2
Uptake of CO
2
by Natural Reservoirs and Global
Carbon Budget
7.3.2.2.1 Ocean-atmosphere
fl
ux
To assess the mean ocean sink, seven methods have been
used. The methods are based on: (1) observations of the partial
pressure of CO
2
at the ocean surface and gas-exchange estimates
(Takahashi et al., 2002); (2) atmospheric inversions based upon
diverse observations of atmospheric CO
2
and atmospheric
transport modelling (see Section 7.2.3.4); (3) observations of
carbon, oxygen, nutrients and chloro
fl
uorocarbons (CFCs) in
seawater, from which the concentration of anthropogenic CO
2
is estimated (Sabine et al., 2004a) combined with estimates of
oceanic transport (Gloor et al., 2003; Mikaloff Fletcher et al.,
2006); (4) estimates of the distribution of water age based on
CFC observations combined with the atmospheric CO
2
history
(McNeil et al., 2003); (5) the simultaneous observations of
the increase in atmospheric CO
2
and decrease in atmospheric
O
2
(Manning and Keeling, 2006); (6) various methods using
observations of change in
13
C in the atmosphere (Ciais et al.,
1995) or the oceans (Gruber and Keeling, 2001; Quay et al.,
2003); and (7) ocean General Circulation Models (Orr et al.,
2001). The ocean uptake estimates obtained with methods (1)
and (2) include in part a
fl
ux component due to the outgassing
of river-supplied inorganic and organic carbon (Sarmiento and
Sundquist, 1992). The magnitude of this necessary correction to
obtain the oceanic uptake
fl
ux of anthropogenic CO
2
is not well
known, as these estimates pertain to the open ocean, whereas
a substantial fraction of the river-induced outgassing likely
occurs in coastal regions. These estimates of the net oceanic
sink are shown in Figure 7.3.
With these corrections, estimates from all methods are
consistent, resulting in a well-constrained global oceanic sink
for anthropogenic CO
2
(see Table 7.1). The uncertainty around
the different estimates is more dif
fi
cult to judge and varies
considerably with the method. Four estimates appear better
constrained than the others. The estimate for the ocean uptake
of atmospheric CO
2
of –2.2 ± 0.5 GtC yr
–1
centred around 1998
based on the atmospheric O
2
/N
2
ratio needs to be corrected
for the oceanic O
2
changes (Manning and Keeling, 2006). The
estimate of –2.0 ± 0.4 GtC yr
–1
centred around 1995 based on
CFC observations provides a constraint from observed physical
transport in the ocean. These estimates of the ocean sink are
shown in Figure 7.6. The mean estimates of –2.2 ± 0.25 and
–2.2 ± 0.2 GtC yr
–1
centred around 1995 and 1994 provide
constraints based on a large number of ocean carbon observations.
These well-constrained estimates all point to a decadal mean
ocean CO
2
sink of –2.2 ± 0.4 GtC yr
–1
centred around 1996,
where the uncertainty is the root mean square of all errors. See
Section 5.4 for a discussion of changes in the ocean CO
2
sink.
7.3.2.2.2 Land-atmosphere
fl
ux
The land-atmosphere CO
2
fl
ux is the sum of the land
use change CO
2
fl
ux (see Section 7.3.2.1) plus sources and
sinks due for instance to legacies of prior land use, climate,
rising CO
2
or N deposition (see Section 7.3.3 for a review of
processes). For assessing the global land-atmosphere
fl
ux, more
than just direct terrestrial observations must be used, because
observations of land ecosystem carbon
fl
uxes are too sparse
and the ecosystems are too heterogeneous to allow global
assessment of the net land
fl
ux with suf
fi
cient accuracy. For
instance, large-scale biomass inventories (Goodale et al., 2002;
UN-ECE/FAO, 2000) are limited to forests with commercial
value, and they do not adequately survey tropical forests. Direct
fl
ux observations by the eddy covariance technique are only
available at point locations, most do not yet have long-term
coverage and they require considerable upscaling to obtain
global estimates (Baldocchi et al., 2001). As a result, two
methods can be used to quantify the net global land-atmosphere
fl
ux: (1) deducing that quantity as a residual between the fossil
fuel and cement emissions and the sum of ocean uptake and
atmospheric increase (Table 7.1), or (2) inferring the land-
atmosphere
fl
ux simultaneously with the ocean sink by inverse
analysis or mass balance computations using atmospheric CO
2
data, with terrestrial and marine processes distinguished using
O
2
/N
2
and/or
13
C observations. Individual estimates of the land-
atmosphere
fl
ux deduced using either method 1 or method 2
Figure 7.6.
Individual estimates of the ocean-atmosphere fl ux reported in Chapter
5 and of the related land-atmosphere fl ux required to close the global carbon bud-
get. The dark thick lines are the revised budget estimates in the AR4 for the 1980s,
the 1990s and the early 2000s, respectively.
520
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
are shown in Figure 7.6. Method 2 was used in the TAR, based
upon O
2
/N
2
data (Langenfelds et al., 1999; Battle et al., 2000).
Corrections have been made to the results of method 2 to
account for the effects of thermal O
2
fl
uxes by the ocean (Le
Quéré et al., 2003). This chapter includes these corrections to
update the 1980s budget, resulting in a land net
fl
ux of –0.3 ±
0.9 GtC yr
–1
during the 1980s. For the 1990s and after, method
1 was adopted for assessing the ocean sink and the land-
atmosphere
fl
ux. Unlike in the TAR, method 1 is preferred for
the 1990s and thereafter (i.e., estimating
fi
rst the ocean uptake,
and then deducing the land net
fl
ux) because the ocean uptake
is now more robustly determined by various oceanographic
approaches (see 7.3.2.2.1) than by the atmospheric O
2
trends.
The numbers are reported in Table 7.1. The land-atmosphere
fl
ux evolved from a small sink in the 1980s of –0.3 ± 0.9
GtC yr
–1
to a large sink during the 1990s of –1.0 ± 0.6 GtC yr
–1
,
and returned to an intermediate value of –0.9 ± 0.6 GtC yr
–1
over
the past
fi
ve years. A recent weakening of the land-atmosphere
uptake has also been suggested by other independent studies of
the
fl
ux variability over the past decades (Jones and Cox, 2005).
The global CO
2
budget is summarised in Table 7.1.
7.3.2.2.3
Residual land sink
In the context of land use change, deforestation dominates
over forest regrowth (see Section 7.3.2.1), and the observed net
uptake of CO
2
by the land biosphere
implies that there must
be an uptake by terrestrial ecosystems elsewhere, called the
‘residual land sink’ (formerly the ‘missing sink’). Estimates
of the residual land sink necessarily depend on the land use
change
fl
ux, and its uncertainty re
fl
ects predominantly the
(large) errors associated with the land use change term. With
the high land use source of Houghton (2003a), the residual
land sink equals –2.3 (–4.0 to –0.3) and –3.2 (–4.5 to –1.9)
GtC yr
–1
respectively for the 1980s and the 1990s. With the
smaller land use source of DeFries et al. (2002), the residual
land sink is –0.9 (–2.0 to –0.3) and –1.9 (–2.9 to –1.0) GtC yr
–1
for the 1980s and the 1990s. Using the mean value of the land
use source from Houghton (2003a) and DeFries et al. (2002) as
reported in Table 7.2, a mean residual land sink of –1.7 (–3.4 to
0.2) and –2.6 (–4.3 to –0.9) GtC yr
–1
for the 1980s and 1990s
respectively is obtained. Houghton (2003a) and DeFries et al.
(2002) give different estimates of the land use source, but they
robustly indicate that deforestation emissions were 0.2 to 0.3
GtC yr
–1
higher in the 1990s than in the 1980s (see Table 7.2).
To compensate for that increase and to match the larger land-
atmosphere uptake during the 1990s, the inferred residual land
sink must have increased by 1 GtC yr
–1
between the 1980s and
the 1990s. This
fi
nding is insensitive to the method used to
determine the land use
fl
ux, and shows considerable decadal
variability in the residual land sink.
7.3.2.2.4
Undisturbed tropical forests: are they a carbon
dioxide sink?
Despite expanding areas of deforestation and degradation,
there are still large areas of tropical forests that are among the
world’s great wilderness areas, with fairly light human impact,
especially in Amazonia. A major uncertainty in the carbon budget
relates to possible net change in the carbon stocks in these forests.
Old growth tropical forests contain huge stores of organic matter,
and are very dynamic, accounting for a major fraction of global
net primary productivity (and about 46% of global biomass;
Brown and Lugo, 1982). Changes in the carbon balance of these
regions could have signi
fi
cant effects on global CO
2
.
Recent studies of the carbon balance of study plots in
mature, undisturbed tropical forests (Phillips et al., 1998;
Baker et al., 2004) report accumulation of carbon at a mean
rate of 0.7 ± 0.2 MgC ha
–1
yr
–1
, implying net carbon uptake
into global Neotropical biomass of 0.6 ± 0.3 GtC yr
–1
. An
intriguing possibility is that rising CO
2
levels could stimulate
this uptake by accelerating photosynthesis, with ecosystem
respiration lagging behind. Atmospheric CO
2
concentration has
increased by about 1.5 ppm (0.4%) yr
–1
, suggesting incremental
stimulation of photosynthesis of about 0.25% (e.g., next year’s
photosynthesis should be 1.0025 times this year’s) (Lin et
al., 1999; Farquhar et al., 2001). For a mean turnover rate of
about 10 years for organic matter in tropical forests, the present
imbalance between uptake of CO
2
and respiration might be
2.5% (1.0025
10
), consistent with the reported rates of live
biomass increase (~3%).
But the recent pan-tropical warming, about 0.26°C per
decade (Malhi and Wright, 2004), could increase water stress
and respiration, and stimulation by CO
2
might be limited by
nutrients (Chambers and Silver, 2004; Koerner, 2004; Lewis
et al., 2005; see below), architectural constraints on how much
biomass a forest can hold, light competition, or ecological shifts
favouring short lived trees or agents of disturbance (insects,
lianas) (Koerner, 2004). Indeed, Baker et al. (2004) note higher
mortality rates and increased prevalence of lianas, and, since dead
organic pools were not measured, effects of increased disturbance
may give the opposite sign of the imbalance inferred from live
biomass only (see, e.g.,
Rice et al., 2004). Methodological
bias associated with small plots, which under-sample natural
disturbance and recovery, might also lead to erroneous inference
of net growth (Koerner, 2004). Indeed, studies involving large-
area plots (9–50 ha) have indicated either no net long-term
change or a long-term net decline in above ground live biomass
(Chave et al., 2003;
Baker et al., 2004; Clark, 2004; Laurance et
al., 2004), and a
fi
ve-year study of a 20 ha plot in Tapajos, Brazil
show increasing live biomass offset by decaying necromass
(Fearnside, 2000; Saleska et al., 2003).
Koerner (2004) argues that accurate assessment of trends in
forest carbon balance requires long-term monitoring of many
replicate plots or very large plots; lacking these studies, the
net carbon balance of undisturbed tropical forests cannot be
authoritatively assessed based on
in situ
studies. If the results
from the plots are extrapolated for illustration, the mean above
ground carbon sink would be 0.89 ± 0.32 MgC ha
–1
yr
–1
(Baker
et al., 2004), or 0.54 ± 0.19 GtC yr
–1
(Malhi and Phillips 2004)
extrapolated to all Neotropical moist forest area (6.0 × 10
6
km
2
).
If the uncompiled data from the African and Asian tropics (50%
of global moist tropical forest area) were to show a similar
trend, the associated tropical live biomass sink would be about
521
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
3
Data can be accessed for instance via the World Data Centre for Greenhouse Gases (http://gaw.kishou.go.jp/wdcgg.html) or the NOAA ESRL Global Monitoring Division (http://
www.cmdl.noaa.gov/ccgg/index.html)
1.2 ± 0.4 GtC yr
–1
, close to balancing the net source due to
deforestation inferred by DeFries et al. (2002) and Achard et al.
(2004)
(Table 7.2).
7.3.2.2.5 New
fi
ndings on the carbon budget
The revised carbon budget in Table 7.1 shows new estimates
of two key numbers. First, the
fl
ux of CO
2
released to the
atmosphere from land use change is estimated to be 1.6 (0.5
to 2.7) GtC yr
–1
for the 1990s. A revision of the TAR estimate
for the 1980s (see TAR, Chapter 3) downwards to 1.4 (0.4 to
2.3) GtC yr
–1
suggests little change between the 1980s and
1990s, but there continues to be considerable uncertainty in
these estimates. Second, the net residual terrestrial sink seems
to have been larger in the 1990s than in the periods before and
after. Thus, a transient increase in terrestrial uptake during the
1990s explains the lower airborne fraction observed during that
period. The ocean uptake has increased by 22% between the
1980s and the 1990s, but the fraction of emissions (fossil plus
land use) taken up by the ocean has remained constant.
7.3.2.3 Regional
Fluxes
Quantifying present-day regional carbon sources and sinks
and understanding the underlying carbon mechanisms are
needed to inform policy decisions. Furthermore, by analysing
spatial and temporal detail, mechanisms can be isolated.
7.3.2.3.1
The top-down view: atmospheric inversions
The atmosphere mixes and integrates surface
fl
uxes that
vary spatially and temporally. The distribution of regional
fl
uxes over land and oceans can be retrieved using observations
of atmospheric CO
2
and related tracers within models of
atmospheric transport. This is called the ‘top-down’ approach
to estimating
fl
uxes. Atmospheric inversions belong to that
approach, and determine an optimal set of
fl
uxes that minimise
the mismatch between modelled and observed concentrations,
accounting for measurement and model errors. Fossil fuel
emissions have small uncertainties that are often ignored and,
when considered (e.g., Enting et al., 1995; Rodenbeck et al.,
2003a), are found to have little in
fl
uence on the inversion.
Fossil fuel emissions are generally considered perfectly known
in inversions, so that their effect can be easily modelled and
subtracted from atmospheric CO
2
data to solve for regional land-
atmosphere and ocean-atmosphere
fl
uxes, although making such
an assumption biases the results (Gurney et al., 2005). Input
data for inversions come from a global network of about 100
CO
2
concentration measurement sites,
3
with mostly discrete
fl
ask sampling, and a smaller number of
in situ
continuous
measurement sites. Generally, regional
fl
uxes derived from
inverse models have smaller uncertainties upwind of regions
with denser data coverage. Measurement and modelling errors
and uneven and sparse coverage of the network generate random
errors in inversion results. In addition, inverse methodological
details, such as the choice of transport model, can introduce
systematic errors. A number of new inversion ensembles, with
different methodological details, have been produced since
the TAR (Gurney et al., 2003; Rödenbeck et al., 2003a,b;
Peylin et al., 2005; Baker et al., 2006). Generally, con
fi
dence
in the long-term mean inverted regional
fl
uxes is lower than
con
fi
dence in the year-to-year anomalies (see Section 7.3.2.4).
For individual regions, continents or ocean basins, the errors of
inversions increase and the signi
fi
cance can be lost. Because of
this, Figure 7.7 reports
the oceans and land
fl
uxes aggregated
into large latitude bands, as well as a breakdown of
fi
ve land
and ocean regions in the NH, which is constrained by denser
atmospheric stations. Both random and systematic errors are
reported in Figure 7.7.
7.3.2.3.2
The bottom-up view: land and ocean observations
and models
The range of carbon
fl
ux and inventory data enables
quanti
fi
cation of the distribution and variability of CO
2
fl
uxes
between the Earth’s surface and the atmosphere. This is called
the ‘bottom-up’ approach. The
fl
uxes can be determined by
measuring carbon stock changes at repeated intervals, from
which time-integrated
fl
uxes can be deduced, or by direct
observations of the
fl
uxes. The stock change approach includes
basin-scale
in situ
measurements of dissolved and particulate
organic and inorganic carbon or tracers in the ocean (e.g.,
Sabine et al., 2004a), extensive forest biomass inventories (e.g.,
UN-ECE/FAO, 2000; Fang et al., 2001; Goodale et al., 2002;
Nabuurs et al., 2003; Shvidenko and Nilsson, 2003) and soil
carbon inventories and models (e.g., Ogle et al., 2003; Bellamy
et al., 2005; van Wesemael et al., 2005; Falloon et al., 2006). The
direct
fl
ux measurement approach includes surveys of ocean CO
2
partial pressure (pCO
2
) from ship-based measurements, drifters
and time series (e.g., Lefèvre et al., 1999; Takahashi et al., 2002),
and ecosystem
fl
ux measurements via eddy covariance
fl
ux
networks (e.g., Valentini et al., 2000; Baldocchi et al., 2001).
The air-sea CO
2
fl
uxes consist of a superposition of natural
and anthropogenic CO
2
fl
uxes, with the former being globally
nearly balanced (except for a small net outgassing associated
with the input of carbon by rivers). Takahashi et al. (2002) present
both surface ocean pCO
2
and estimated atmosphere-ocean CO
2
fl
uxes (used as prior knowledge in many atmospheric inversions)
normalised to 1995 using National Centers for Environmental
Prediction (NCEP)/National Center for Atmospheric Research
(NCAR) 41-year mean monthly winds. Large annual CO
2
fl
uxes to the ocean occur in the Southern Ocean subpolar
regions (40°S–60°S), in the North Atlantic poleward of 30°N
and in the North Paci
fi
c poleward of 30°N (see Figure 7.8).
Ocean inversions calculate natural and anthropogenic air-sea
fl
uxes (Gloor et al., 2003; Mikaloff Fletcher et al., 2006), by
optimising ocean carbon model results against vertical pro
fi
les
of DIC data. These studies indicate that the Southern Ocean is
the largest sink of anthropogenic CO
2
, together with mid- to
high-latitude regions in the North Atlantic. This is consistent
with global ocean hydrographic surveys (Sabine et al., 2004a
522
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
and Figure 5.10). However, only half of the
anthropogenic CO
2
absorbed by the Southern
Ocean is stored there, due to strong northward
transport (Mikaloff Fletcher et al., 2006). The
tropical Paci
fi
c is a broad area of natural CO
2
outgassing to the atmosphere, but this region is
a sink of anthropogenic CO
2
.
Models are used to extrapolate
fl
ux
observations into regional estimates, using
remote-sensing properties and knowledge of
the processes controlling the CO
2
fl
uxes and
their variability. Rayner et al. (2005) use inverse
process-based models, where observations are
‘assimilated’ to infer optimised
fl
uxes. Since
the TAR, the global air-sea
fl
ux synthesis
has been updated (Takahashi et al., 2002 and
Figure 7.8), and new syntheses have been made
of continental-scale carbon budgets of the
NH continents (Pacala et al., 2001; Goodale
et al., 2002; Janssens et al., 2003; Shvidenko
and Nilsson, 2003; Ciais et al., 2005a), and of
tropical forests (Malhi and Grace, 2000). These
estimates are shown in Figure 7.7 and compared
with inversion results.
Comparing bottom-up regional
fl
uxes
with inversion results is not straightforward
because: (1) inversion
fl
uxes may contain a
certain amount of prior knowledge of bottom-
up
fl
uxes so that the two approaches are not
fully independent; (2) the time period for which
inversion models and bottom-up estimates
are compared is often not consistent, in the
presence of interannual variations in
fl
uxes
4
(see Section 7.3.2.4); and (3) inversions of
CO
2
data produce estimates of CO
2
fl
uxes, so
the results will differ from budgets for carbon
fl
uxes (due to the emission of reduced carbon
compounds that get oxidized into CO
2
in the
atmosphere and are subject to transport and
chemistry) and carbon storage changes (due
to lateral carbon transport, e.g., by rivers)
(Sarmiento and Sundquist, 1992). Some of these effects can be
included by ‘off-line’ conversion of inversion results (Enting
and Mansbridge, 1991; Suntharalingam et al., 2005). Reduced
carbon compounds such as volatile organic compounds (VOCs),
carbon monoxide (CO) and CH
4
emitted by ecosystems and
human activities are transported and oxidized into CO
2
in the
atmosphere (Folberth et al., 2005). Trade of forest and crop
products displaces carbon from ecosystems (Imhoff et al.,
2004). Rivers displace dissolved and particulate inorganic and
organic carbon from land to ocean (e.g., Aumont et al., 2001).
A summary of the main results of inversion and bottom-up
estimates of regional CO
2
fl
uxes is given below.
7.3.2.3.3
Robust
fi
ndings of regional land-atmosphere
fl
ux
•
Tropical lands are found in inversions to be either carbon
neutral or sink regions, despite widespread deforestation,
as is apparent in Figure 7.7, where emissions from land
include deforestation. This implies carbon uptake by
undisturbed tropical ecosystems, in agreement with limited
forest inventory data in the Amazon (Phillips et al., 1998;
Malhi and Grace, 2000).
•
Inversions place a substantial land carbon sink in the NH.
The inversion estimate is –1.7 (–0.4 to –2.3) GtC yr
–1
(from
data in Figure 7.7). A bottom-up value of the NH land
sink of –0.98 (–0.38 to –1.6) GtC yr
–1
was also estimated,
4
For instance, the chosen 1992 to 1996 time period for assessing inversion fl uxes, dictated by the availability of the Atmospheric Tracer Transport Model Intercomparison Project
(TransCom 3) intercomparison results (Gurney et al., 2002, 2003, 2004), corresponds to a low growth rate and to a stronger terrestrial carbon sink, likely due to the eruption of Mt.
Pinatubo.
Figure 7.7.
Regional ocean-atmosphere and land-atmosphere CO
2
fl uxes for the NH (top) and the globe
(bottom) from inversion ensembles and bottom-up studies. Fluxes to the atmosphere are positive and
uptake has a negative sign. Inversion results all correspond to the post-Pinatubo period 1992 to 1996.
Orange: Bottom-up terrestrial fl uxes from Pacala et al. (2001) and Kurz and Apps (1999) for North America,
from Janssens et al. (2003) for Europe and from Shvidenko and Nilsson (2003) plus Fang et al. (2001) for
North Asia (Asian Russia and China). Cyan (fi lled circles): Bottom-up ocean fl ux estimates from Takahashi,
et al. (2002). Blue: ocean fl uxes from atmospheric inversions. Green: terrestrial fl uxes from inversion
models. Magenta: total inversion fl uxes. Red: fossil fuel emissions. The mean fl ux of different inversion
ensembles is reported. Inversion errors for regional fl uxes are not reported here; their values usually range
between 0.5 and 1 GtC yr
–1
. Error bar: range of atmospheric inversion fl uxes from the TAR. Squares: Gurney
et al. (2002) inversions using annual mean CO
2
observations and 16 transport models. Circles: Gurney et al.
(2003) inversions using monthly CO
2
observations and 13 transport models. Triangles: Peylin et al. (2005)
inversions with three transport models, three regional breakdowns and three inversion settings. Inverted
triangles: Rödenbeck et al. (2003a) inversions where the fl uxes are solved on the model grid using monthly
fl ask data.
523
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Figure 7.8.
Estimates (4° × 5°) of sea-to-air fl ux of CO
2
, computed using 940,000 measurements of
surface water pCO
2
collected since 1956 and averaged monthly, together with NCEP/NCAR 41-year mean
monthly wind speeds and a (10-m wind speed)
2
dependence on the gas transfer rate (Wanninkhof, 1992).
The fl uxes were normalised to the year 1995 using techniques described in Takahashi et al. (2002), who
used wind speeds taken at the 0.995 standard deviation level (about 40 m above the sea surface). The an-
nual fl ux of CO
2
for 1995 with 10-m winds is –1.6 GtC yr
–1
, with an approximate uncertainty (see Footnote
1) of ±1 GtC yr
–1
, mainly due to uncertainty in the gas exchange velocity and limited data coverage. This
estimated global fl ux consists of an uptake of anthropogenic CO
2
of –2.2 GtC yr
–1
(see text) plus an outgas-
sing of 0.6 GtC yr
–1
, corresponding primarily to oxidation of organic carbon borne by rivers (Figure 7.3).
The monthly fl ux values with 10-m winds used here are available from T. Takahashi at http://www.ldeo.
columbia.edu/res/pi/CO2/carbondioxide/pages/air_sea_fl ux_rev1.html.
based upon regional synthesis studies
(Kurz and Apps, 1999; Fang et al., 2001;
Pacala et al., 2001; Janssens et al., 2003;
Nilsson et al., 2003; Shvidenko and
Nilsson, 2003). The inversion sink value
is on average higher than the bottom-up
value. Part of this discrepancy could be
explained by lateral transport of carbon
via rivers, crop trade and emission of
reduced carbon compounds.
•
The longitudinal partitioning of the
northern land sink between North
America, Europe and Northern Asia
has large uncertainties (see Figure 7.7).
Inversions give a very large spread over
Europe (–0.9 to +0.2 GtC yr
–1
), and
Northern Asia (–1.2 to +0.3 GtC yr
–1
)
and a large spread over North America
(–0.6 to –1.1 GtC yr
–1
). Within the
uncertainties of each approach,
continental-scale carbon
fl
uxes from
bottom-up and top-down methods over
Europe, North America and Northern
Asia are mutually consistent (Pacala
et al., 2001; Janssens et al., 2003). The
North American carbon sink estimated
by recent inversions is on average lower
than an earlier widely cited study by Fan et al. (1998).
Nevertheless, the Fan et al. (1998) estimate remains
within the range of inversion uncertainties. In addition,
the
fl
uxes calculated in Fan et al. (1998) coincide with the
low growth rate post-Pinatubo period, and hence are not
necessarily representative of long-term behaviour.
7.3.2.3.4 Robust
fi
ndings of regional ocean-atmosphere
fl
ux
•
The regional air-sea CO
2
fl
uxes consist of a superposition
of natural and anthropogenic CO
2
fl
uxes, with the former
being globally nearly balanced (except for a small net
outgassing associated with the input of carbon by rivers),
and the latter having a global integral uptake of 2.2 ± 0.5
GtC yr
–1
(see Table 7.1).
•
The tropical oceans are outgassing CO
2
to the atmosphere
(see Figure 7.8), with a mean
fl
ux of the order of 0.7
GtC yr
–1
, estimated from an oceanic inversion (Gloor et
al., 2003), in good agreement with atmospheric inversions
(0 to 1.5 GtC yr
–1
), and estimates based on oceanic pCO
2
observations (0.8 GtC yr
–1
; Takahashi et al., 2002).
•
The extratropical NH ocean is a net sink for anthropogenic
and natural CO
2
, with a magnitude of the order of 1.2
GtC yr
–1
, consistent among various estimates.
•
The Southern Ocean is a large sink of atmospheric CO
2
(Takahashi et al., 2002; Gurney et al., 2002) and of
anthropogenic CO
2
(Gloor et al., 2003; Mikaloff Fletcher et
al., 2006). Its magnitude has been estimated to be about 1.5
GtC yr
–1
. This estimate is consistent among the different
methods at the scale of the entire Southern Ocean. However,
differences persist with regard to the Southern Ocean
fl
ux
distribution between subpolar and polar latitudes (T. Roy et
al., 2003). Atmospheric inversions and oceanic inversions
indicate a larger sink in subpolar regions (Gurney et al.,
2002; Gloor et al., 2003), consistent with the distribution of
CO
2
fl
uxes based on available
Δ
pCO
2
observations (Figure
7.8 and Takahashi, 2002).
7.3.2.4
Interannual Changes in the Carbon Cycle
7.3.2.4.1
Interannual changes in global
fl
uxes
The atmospheric CO
2
growth rate exhibits large interannual
variations (see Figure 3.3, the TAR and http://lgmacweb.env.
uea.ac.uk/lequere/co2/carbon_budget). The variability of fossil
fuel emissions and the estimated variability in net ocean uptake
are too small to account for this signal, which must be caused
by year-to-year
fl
uctuations in land-atmosphere
fl
uxes. Over the
past two decades, higher than decadal-mean CO
2
growth rates
occurred in 1983, 1987, 1994 to 1995, 1997 to 1998 and 2002
to 2003. During such episodes, the net uptake of anthropogenic
CO
2
(sum of land and ocean sinks) is temporarily weakened.
Conversely, small growth rates occurred in 1981, 1992 to 1993
and 1996 to 1997, associated with enhanced uptake. Generally,
high CO
2
growth rates correspond to El Niño climate conditions,
and low growth rates to La Niña (Bacastow and Keeling, 1981;
Lintner, 2002). However, two episodes of CO
2
growth rate
variations during the past two decades did not re
fl
ect such
an El Niño forcing. In 1992 to 1993, a marked reduction in
growth rate occurred, coincident with the cooling and radiation
524
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
anomaly caused by the eruption of Mt. Pinatubo in June 1991.
In 2002 to 2003, an increase in growth rate occurred, larger
than expected based on the very weak El Niño event (Jones and
Cox, 2005). It coincided with droughts in Europe (Ciais et al.,
2005b), in North America (Breshears et al., 2005) and in Asian
Russia (IFFN, 2003).
S
ince the TAR, many studies have con
fi
rmed that the
variability of CO
2
fl
uxes is mostly due to land
fl
uxes, and that
tropical lands contribute strongly to this signal (Figure 7.9). A
predominantly terrestrial origin of the growth rate variability can
be inferred from (1) atmospheric inversions assimilating time
series of CO
2
concentrations from different stations (Bousquet
et al., 2000; Rödenbeck et al., 2003b; Baker et al., 2006),
(2) consistent relationships between
δ
13
C and CO
2
(Rayner et al.,
1999), (3) ocean model simulations (e.g., Le Quéré et al., 2003;
McKinley et al., 2004a) and (4) terrestrial carbon cycle and
coupled model simulations (e.g., C. Jones et al., 2001; McGuire
et al., 2001; Peylin et al., 2005; Zeng et al., 2005). Currently,
there is no evidence for basin-scale interannual variability of the
air-sea CO
2
fl
ux exceeding ±0.4 GtC yr
–1
, but there are large
ocean regions, such as the Southern Ocean, where interannual
variability has not been well observed.
7.3.2.4.2
Interannual variability in regional
fl
uxes,
atmospheric inversions and bottom-up models
Year-to-year
fl
ux anomalies can be more robustly inferred
by atmospheric inversions than mean
fl
uxes. Yet, at the scale
of continents or ocean basins, the inversion errors increase
and the statistical signi
fi
cance of the inferred regional
fl
uxes
decreases.
5
This is why Figure 7.9 shows the land-atmosphere
and ocean-atmosphere
fl
ux anomalies over broad latitude
bands only for the inversion ensembles of Baker et al. (2006),
Bousquet et al. (2000) and Rödenbeck et al. (2003b). An
important
fi
nding of these studies is that differences in transport
models have little impact on the interannual variability of
fl
uxes. Interannual variability of global land-atmosphere
fl
uxes (±4 GtC yr
–1
between extremes) is larger than that of
air-sea
fl
uxes and dominates the global
fl
uxes. This result is
also true over large latitude bands (Figure 7.9). Tropical land
fl
uxes exhibit on average a larger variability than temperate
and boreal
fl
uxes. Inversions give tropical land
fl
ux anomalies
of the order of ±1.5 to 2 GtC yr
–1
, which compare well in
timing and magnitude with terrestrial model results (Tian
et al., 1998; Peylin et al., 2005; Zeng et al., 2005). In these
studies, enhanced sources occur during El Niño episodes and
abnormal sinks during La Niña. In addition to the in
fl
uence of
these climate variations on ecosystem processes (Gérard et al.,
1999; C. Jones et al., 2001), regional droughts during El Niño
events promote large biomass
fi
res, which appear to contribute
to high
CO
2
growth rates during the El Niño episodes (Barbosa
et al., 1999; Langenfelds et al., 2002; Page et al., 2002; van
der Werf et al., 2003, 2004; Patra et al., 2005).
Inversions robustly attribute little variability to ocean-
atmosphere CO
2
fl
ux (±0.5 GtC yr
–1
between extremes), except
for the recent work of Patra et al. (2005). This is in agreement with
ocean model and ocean observations (Lee et al., 1998; Le Quéré
et al., 2003; Obata and Kitamura, 2003; McKinley et al., 2004b).
However, inversions and ocean models differ on the dominant
geographic contributions to the variability. Inversions estimate
similar variability in both hemispheres, whereas ocean models
estimate more variability in the Southern Ocean (Bousquet et
al., 2000; Rödenbeck et al., 2003b; Baker et al., 2006). Over the
North Atlantic, Gruber et al. (2002) suggest a regional CO
2
fl
ux
variability (extremes of ±0.3 GtC yr
–1
) by extrapolating data
from a single ocean station, but McKinley et al. (2004a,b) model
a small variability (extremes of ±0.1 GtC yr
–1
). The equatorial
Paci
fi
c is the ocean region of the world where the variability
is constrained with repeated
Δ
pCO
2
observations (variations of
about ±0.4 GtC yr
–1
; Feely et al., 2002), with a reduced source
of CO
2
during El Niño associated with decreased upwelling of
CO
2
-rich waters. Over this region, some inversion results (e.g.,
Bousquet et al., 2000) compare well in magnitude and timing
with ocean and coupled model results (Le Quéré et al., 2000;
C. Jones et al., 2001; McKinley et al., 2004a,b) and with
Δ
pCO
2
observations (Feely et al., 1999, 2002).
7.3.2.4.3
Slowdown in carbon dioxide growth rates during
the early 1990s
The early 1990s had anomalously strong global sinks for
atmospheric CO
2
, compared with the decadal mean (Table 7.1).
Although a weak El Niño from 1991 to 1995 may have helped
to enhance ocean uptake at that time, inversions and O
2
:N
2
and
δ
13
C-CO
2
atmospheric data (Battle et al., 2000) indicate that the
enhanced uptake was of predominantly terrestrial origin. The
regions where the 1992 to 1993 abnormal sink is projected to be
are not robustly estimated by inversions. Both Bousquet et al.
(2000) and Rödenbeck et al. (2003b) project a large fraction of
that sink in temperate North America, while Baker et al. (2006)
place it predominantly in the tropics. Model results suggest
that cooler temperatures caused by the Mt. Pinatubo eruption
reduced soil respiration and enhanced NH carbon uptake (Jones
and Cox, 2001b; Lucht et al., 2002), despite lower productivity
as indicated by remote sensing of vegetation activity. In
addition, aerosols from the volcanic eruption scattered sunlight
and increased its diffuse fraction, which is used more ef
fi
ciently
by plant canopies in photosynthesis than direct light (Gu et
al., 2003). It has been hypothesised that a transient increase
in the diffuse fraction of radiation enhanced CO
2
uptake by
land ecosystems in 1992 to 1993, but the global signi
fi
cance
and magnitude of this effect remains unresolved (Roderick et
al., 2001; Krakauer and Randerson, 2003; Angert et al., 2004;
Robock, 2005).
5
In other words, the model bias has only a small infl uence on inversions of interannual variability. These interannual inversion studies all report a random error and a systematic
error range derived from sensitivity tests with different settings. Bousquet et al. (2000) used large regions and different inversion settings for the period 1980 to 1998. Rödenbeck
et al. (2003) used one transport model and inverted fl uxes at the resolution of the model grid for the period 1982 to 2002, with different inversion settings. Baker et al. (2006) used
large regions but 13 different transport models for the period 1988 to 2002.
525
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Figure 7.9.
Year-to-year anomalies in ocean-atmosphere and land-atmosphere CO
2
fl uxes (GtC yr
–1
) from interannual inversion ensembles covering the past 20 years or so,
grouped into large latitude bands, and over the globe. Three different inversion ensembles from Bousquet et al. (2000), Rödenbeck et al. (2003a) and Baker et al. (2006) are
shown. For each fl ux and each region, the anomalies were obtained by subtracting the long-term mean fl ux and removing the seasonal signal. Grey shaded regions indicate El
Niño episodes, and the black bars indicate the cooling period following the Mt. Pinatubo eruption.
526
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.3.2.4.4
Speed-up in carbon dioxide growth rates during
the late 1990s
The high CO
2
growth in 1998 coincided with a global
increase in CO concentrations attributable to wild
fi
res
(Yurganov et al., 2005) in Southeast Asia (60%), South America
(30%) and Siberia (van der Werf et al., 2004). Langenfelds et al.
(2002) analyse the correlations in the interannual growth rate
of CO
2
and other species at 10 stations and link the 1997 to
1998 (and the 1994 to 1995) anomalies to high
fi
re emissions
as a single process. Achard et al. (2004) estimate a source of
0.88 ± 0.07 GtC emitted from the burning of 2.4 × 10
6
ha of
peatland in the Indonesian forest
fi
res in 1997 to 1998, and Page
et al. (2002) estimate a source of +0.8 to +2.6 GtC. During the
1997 to 1998 high CO
2
growth rate episode, inversions place
an abnormal source over tropical Southeast Asia, in good
agreement with such bottom-up evidence. The relationship
between El Niño and CO
2
emissions from
fi
res is not uniform:
fi
re emissions from low productivity ecosystems in Africa and
northern Australia are limited by fuel load density and thus
decrease during drier periods, in contrast to the response in
tropical forests (Barbosa et al., 1999; Randerson et al., 2005).
In addition, co-varying processes such as reduced productivity
caused by drought in tropical forests during El Niño episodes
may be superimposed on
fi
re emissions. From 1998 to 2003,
extensive drought in mid-latitudes of the NH (Hoerling and
Kumar, 2003), accompanied by more wild
fi
res in some regions
(Balzter et al., 2005; Yurganov et al., 2005) may have led to
decreased photosynthesis and carbon uptake (Angert et al.,
2005; Ciais et al., 2005b), helping to increase the atmospheric
CO
2
growth rate.
7.3.3
Terrestrial Carbon Cycle Processes and
Feedbacks to Climate
The net exchange of carbon between the terrestrial biosphere
and the atmosphere is the difference between carbon uptake by
photosynthesis and release by plant respiration, soil respiration
and disturbance processes (
fi
re, windthrow, insect attack and
herbivory in unmanaged systems, together with deforestation,
afforestation, land management and harvest in managed
systems). Over at least the last 30 years, the net result of all these
processes has been uptake of atmospheric CO
2
by terrestrial
ecosystems (Table 7.1, ‘land-atmosphere
fl
ux’ row). It is critical
to understand the reasons for this uptake and its likely future
course. Will uptake by the terrestrial biosphere grow or diminish
with time, or even reverse so that the terrestrial biosphere
becomes a net source of CO
2
to the atmosphere? To answer this
question it is necessary to understand the underlying processes
and their dependence on the key drivers of climate, atmospheric
composition and human land management.
Drivers that affect the carbon cycle in terrestrial
ecosystems can be classi
fi
ed as (1) direct climate effects
(changes in precipitation, temperature and radiation regime);
(2) atmospheric composition effects (CO
2
fertilization, nutrient
deposition, damage by pollution); and (3) land use change
effects (deforestation, afforestation, agricultural practices, and
their legacies over time). This section
fi
rst summarises current
knowledge of the processes by which each of these drivers
in
fl
uence the terrestrial carbon balance, and then examines
knowledge of the integrative consequences of all these processes
in the key case of tropical forests.
7.3.3.1
Processes Driven by Climate, Atmospheric
Composition and Land Use Change
7.3.3.1.1
Climatic regulation of terrestrial carbon exchange
Ecosystem responses to environmental drivers (sunlight,
temperature, soil moisture) and to ecological factors (e.g., forest
age, nutrient supply, organic substrate availability; see, e.g.,
Clark, 2002; Ciais et al., 2005b; Dunn et al., 2007) are complex.
For example, elevated temperature and higher soil water content
enhance rates for heterotrophic respiration in well-aerated soils,
but depress these rates in wet soils. Soil warming experiments
typically show marked soil respiration increases at elevated
temperature (Oechel et al., 2000; Rustad et al., 2001; Melillo
et al., 2002), but CO
2
fl
uxes return to initial levels in a few
years as pools of organic substrate re-equilibrate with inputs
(Knorr et al., 2005). However, in dry soils, decomposition may
be limited by moisture and not respond to temperature (Luo et
al., 2001). Carbon cycle simulations need to capture both the
short- and long-term responses to changing climate to predict
carbon cycle responses.
Current models of terrestrial carbon balance have dif
fi
culty
simulating measured carbon
fl
uxes over the full range of temporal
and spatial scales, including instantaneous carbon exchanges at
the leaf, plot or ecosystem level, seasonal and annual carbon
fl
uxes at the stand level and decadal to centennial accumulation
of biomass and organic matter at stand or regional scales (Melillo
et al., 1995; Thornton et al., 2002). Moreover, projections of
changes in land carbon storage are tied not only to ecosystem
responses to climate change, but also to the modelled projections
of climate change itself. As there are strong feedbacks between
these components of the Earth system (see Section 7.3.5), future
projections must be considered cautiously.
7.3.3.1.2
Effects of elevated carbon dioxide
On physiological grounds, almost all models predict
stimulation of carbon assimilation and sequestration in response
to rising CO
2
, called ‘CO
2
fertilization’ (Cramer et al., 2001;
Oren et al., 2001; Luo et al., 2004; DeLucia et al., 2005). Free Air
CO
2
Enrichment (FACE) and chamber studies have been used
to examine the response of ecosystems to large (usually about
50%) step increases in CO
2
concentration. The results have been
variable (e.g., Oren et al., 2001; Nowak et al., 2004; Norby et
al., 2005). On average, net CO
2
uptake has been stimulated,
but not as much as predicted by some models. Other factors
(e.g., nutrients or genetic limitations on growth) can limit plant
growth and reduce response to CO
2
. Eleven FACE experiments,
encompassing bogs, grasslands, desert and young temperate
tree stands report an average increased net primary productivity
(NPP) of 12% when compared to ambient CO
2
levels (Nowak
et al., 2004). There is a large range of responses, with woody
527
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
plants consistently showing NPP increases of 23 to 25%
(Norby et al., 2005), but much smaller increases for grain crops
(Ainsworth and Long, 2005), re
fl
ecting differential allocation
of the incremental organic matter to shorter- vs. longer-lived
compartments. Overall, about two-thirds of the experiments
show positive response to increased CO
2
(Ainsworth and Long,
2005; Luo et al., 2005). Since saturation of CO
2
stimulation due
to nutrient or other limitations is common (Dukes et al., 2005;
Koerner et al., 2005), it is not yet clear how strong the CO
2
fertilization effect actually is.
7.3.3.1.3
Nutrient and ozone limitations to carbon
sequestration
The basic biochemistry of photosynthesis implies
that stimulation of growth will saturate under high CO
2
concentrations and be further limited by nutrient availability
(Dukes et al., 2005; Koerner et al., 2005) and by possible
acclimation of plants to high CO
2
levels (Ainsworth and
Long, 2005). Carbon storage by terrestrial plants requires
net assimilation of nutrients, especially N, a primary limiting
nutrient at middle and high latitudes and an important nutrient
at lower latitudes (Vitousek et al., 1998). Hungate et al. (2003)
argue that ‘soil C sequestration under elevated CO
2
is constrained
both directly by N availability and indirectly by nutrients
needed
to support N
2
fi
xation’, and Reich et al. (2006) conclude that
‘soil N supply is probably an important constraint on global
terrestrial responses to elevated CO
2
’. This view appears to be
consistent with other recent studies (e.g., Finzie et al., 2006;
Norby et al., 2006; van Groenigen et al., 2006) and with at least
some of the FACE data, further complicating estimation of the
current effects of rising CO
2
on carbon sequestration globally.
Additional N supplied through atmospheric deposition or
direct fertilization can stimulate plant growth (Vitousek, 2004)
and in principle could relieve the nutrient constraint on CO
2
fertilization. Direct canopy uptake of atmospheric N may be
particularly effective (Sievering et al., 2000). Overall, the
effectiveness of N inputs appears to be limited by immobilisation
and other mechanisms. For example, when labelled nitrogen
(
15
N) was added to soil and litter in a forest over seven
years, only a small fraction became available for tree growth
(Nadelhoffer et al., 2004). Moreover, atmospheric N deposition
is spatially correlated with air pollution, including elevated
atmospheric ozone. Ozone and other pollutants may have
detrimental effects on plant growth, possibly further limiting
the stimulation of carbon uptake by anthropogenic N emissions
(Ollinger and Aber, 2002; Holland and Carroll, 2003). Indeed,
Felzer et al. (2004) estimate that surface ozone increases since
1950 may have reduced CO
2
sequestration in the USA by 18 to
20 TgC yr
–1
. The current generation of coupled carbon-climate
models (see Section 7.3.5) does not include nutrient limitations
or air pollution effects.
7.3.3.1.4 Fire
Fire is a major agent for conversion of biomass and soil
organic matter to CO
2
(Randerson et al., 2002a–d; Cochrane,
2003; Nepstad et al., 2004; Jones and Cox, 2005; Kasischke et
al., 2005; Randerson et al., 2005). Globally, wild
fi
res (savannah
and forest
fi
res, excluding biomass burning for fuel and land
clearing) oxidize 1.7 to 4.1 GtC yr
–1
(Mack et al., 1996; Andreae
and Merlet, 2001), or about 3 to 8% of total terrestrial NPP.
There is an additional large enhancement of CO
2
emissions
associated with
fi
res stimulated by human activities, such as
deforestation and tropical agricultural development. Thus,
there is a large potential for future alteration in the terrestrial
carbon balance through altered
fi
re regimes. A striking example
occurred during the 1997 to 1998 El Niño, when large
fi
res in
the Southeast Asian archipelago are estimated to have released
0.8 to 2.6 GtC (see Section 7.3.2.4). Fire frequency and intensity
are strongly sensitive to climate change and variability, and
to land use practices. Over the last century, trends in burned
area have been largely driven by land use practices, through
fi
re suppression policies in mid-latitude temperate regions and
increased use of
fi
re to clear forest in tropical regions (Mouillot
and Field, 2005). However, there is also evidence that climate
change has contributed to an increase in
fi
re frequency in
Canada (Gillett et al., 2004). The decrease in
fi
re frequency in
regions like the USA and Europe has contributed to the land
carbon sink there, while increased
fi
re frequency in regions like
Amazonia, Southeast Asia and Canada has contributed to the
carbon source. At high latitudes, the role of
fi
re appears to have
increased in recent decades:
fi
re disturbance in boreal forests
was higher in the 1980s than in any previous decade on record
(Kurz et al., 1995; Kurz and Apps, 1999; Moulliot and Field,
2005). Flannigan et al. (2005) estimate that in the future, the
CO
2
source from
fi
re will increase.
7.3.3.1.5
Direct effects of land use and land management
Evolution of landscape structure, including woody
thickening:
Changes in the structure and distribution of
ecosystems are driven in part by changes in climate and
atmospheric CO
2
, but also by human alterations of landscapes
through land management and the introduction of invasive
species and exotic pathogens. The single most important process
in the latter category is woody encroachment or vegetation
thickening, the increase in woody biomass occurring in (mainly
semi-arid) grazing lands. In many regions, this increase arises
from
fi
re suppression and associated grazing management
practices, but there is also a possibility that increases in CO
2
are giving C
3
woody plants a competitive advantage over C
4
grasses (Bond et al., 2003). Woody encroachment could account
for as much as 22 to 40% of the regional carbon sink in the
USA (Pacala et al., 2001), and a high proportion in northeast
Australia (Burrows et al., 2002). Comprehensive data are
lacking to de
fi
ne this effect accurately.
Deforestation:
Forest clearing (mainly in the tropics) is a
large contributor to the land use change component of the
current atmospheric CO
2
budget, accounting for up to one-third
of total anthropogenic emissions (see Table 7.2; Section 7.3.2.1;
also Table 7.1, row ‘land use change
fl
ux’). The future evolution
of this term in the CO
2
budget is therefore of critical importance.
Deforestation in Africa, Asia and the tropical Americas is
expected to decrease towards the end of the 21st century to a
528
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
small fraction of the levels in 1990 (IPCC, 2000). The declines
in Asia and Africa are driven by the depletion of forests, while
trends in the Americas have the highest uncertainty given the
extent of the forest resource.
Afforestation:
Recent (since 1970) afforestation and
reforestation as direct human-induced activities have not yet
had much impact on the global terrestrial carbon sink. However,
regional sinks have been created in areas such as China, where
afforestation since the 1970s has sequestered 0.45 GtC (Fang et
al., 2001). The largest effect of afforestation is not immediate
but through its legacy.
Agricultural practices:
Improvement of agricultural
practices on carbon-depleted soils has created a carbon sink.
For instance, the introduction of conservation tillage in the
USA is estimated to have increased soil organic matter (SOM)
stocks by about 1.4 GtC over the last 30 years. However, yearly
increases in SOM can be sustained only for 50 to 100 years, after
which the system reaches a new equilibrium (Cole et al., 1996;
Smith et al., 1997). Moreover, modern conservation tillage
often entails large inputs of chemicals and fertilizer, which are
made using fossil fuels, reducing the CO
2
bene
fi
t from carbon
sequestration in agricultural soils. The increase in soil carbon
stocks under low-tillage systems may also be mostly a topsoil
effect with little increase in total pro
fi
le carbon storage observed,
confounded by the fact that most studies of low-tillage systems
have only sampled the uppermost soil layers.
7.3.3.1.6 Forest
regrowth
Some studies suggest that forest regrowth could be a major
contributor to the global land carbon sink (e.g., Pacala et al.,
2001; Schimel et al., 2001; Hurtt et al., 2002). Forest areas
generally increased during the 20th century at middle and
high latitudes (unlike in the tropics). This surprising trend
re
fl
ects the intensi
fi
cation of agriculture and forestry. Globally,
more food is being grown on less land, re
fl
ecting mechanisation
of agriculture, increased fertilizer use and adoption of high-
yield cultivars, although in parts of Africa and Asia the
opposite is occurring. Likewise, intensive forest management
and agroforestry produce more
fi
bre on less land; improved
forest management favours more rapid regrowth of forests
after harvest. These trends have led to carbon sequestration
by regrowing forests. It should be noted, however, that
industrialised agriculture and forestry require high inputs of
fossil energy, so it is dif
fi
cult to assess the net global effects
of agricultural intensi
fi
cation on atmospheric greenhouse gases
and radiative forcing.
Regional studies have con
fi
rmed the plausibility of strong
mid-latitude sinks due to forest regrowth. Data from the eddy
fl
ux tower network show that forests on long-abandoned former
agricultural lands (Curtis et al., 2002) and in industrial managed
forests (Hollinger et al., 2002) take up signi
fi
cant amounts of
carbon every year. Analysis of forest inventory data shows
that, in aggregate, current forest lands are signi
fi
cant sinks for
atmospheric CO
2
(Pacala et al., 2001). Few old growth forests
remain at mid-latitudes (most forests are less than 70 years
old), in part due to forest management. Therefore, forests in
these areas are accumulating biomass because of their ages
and stages of succession. Within wide error bands (see Section
7.3.2.3), the uptake rates inferred from
fl
ux towers are generally
consistent with those inferred from inverse methods (e.g., Hurtt
et al., 2002). Stocks of soil carbon are also likely increasing due
to replenishment of soil organic matter and necromass depleted
during the agricultural phase, and changes in soil microclimate
associated with reforestation; these effects might add 30 to 50%
to the quantity of CO
2
sequestered (e.g., Barford et al., 2001).
It is important to note that at least some of this sequestration
is ‘re
fi
lling’ the de
fi
cits in biomass and soil organic matter,
accumulated in previous epochs (see Figure 7.3), and the
associated CO
2
uptake should be expected to decline in the
coming decades unless sustained by careful management
strategies designed to accomplish that purpose.
7.3.4
Ocean Carbon Cycle Processes and
Feedbacks to Climate
7.3.4.1 Overview of the Ocean Carbon Cycle
Oceanic carbon exists in several forms: as DIC, DOC,
and particulate organic carbon (POC) (living and dead) in an
approximate ratio DIC:DOC:POC = 2000:38:1 (about 37,000
GtC DIC: Falkowski et al., 2000 and Sarmiento and Gruber,
2006; 685 GtC DOC: Hansell and Carlson, 1998; and 13 to 23
GtC POC: Eglinton and Repeta, 2004). Before the industrial
revolution, the ocean contained about 60 times as much carbon
as the atmosphere and 20 times as much carbon as the terrestrial
biosphere/soil compartment.
Seawater can, through inorganic processes, absorb large
amounts of CO
2
from the atmosphere, because CO
2
is a weakly
acidic gas and the minerals dissolved in the ocean have over
geologic time created a slightly alkaline ocean (surface pH 7.9
to 8.25: Degens et al., 1984; Royal Society, 2005). The air-sea
exchange of CO
2
is determined largely by the air-sea gradient in
pCO
2
between atmosphere and ocean. Equilibration of surface
ocean and atmosphere occurs on a time scale of roughly one year.
Gas exchange rates increase with wind speed (Wanninkhof and
McGillis, 1999; Nightingale et al., 2000) and depend on other
factors such as precipitation, heat
fl
ux, sea ice and surfactants.
The magnitudes and uncertainties in local gas exchange rates
are maximal at high wind speeds. In contrast, the equilibrium
values for partitioning of CO
2
between air and seawater and
associated seawater pH values are well established (Zeebe and
Wolf-Gladrow, 2001; see Box 7.3).
In addition to changes in advection and mixing, the ocean
can alter atmospheric CO
2
concentration through three
mechanisms (Volk and Hoffert, 1985), illustrated in Figure 7.10:
(1) absorption or release of CO
2
due to changes in solubility of
gaseous CO
2
(‘solubility pump’); (2) changes in carbon
fi
xation
to POC in surface waters by photosynthesis and export of this
carbon through sinking of organic particles out of the surface
layer (‘organic carbon pump’) – this process is limited to
fi
rst
order by availability of light and nutrients (phosphate, nitrate,
silicic acid and micronutrients such as iron); and (3) changes in
529
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Box 7.3: Marine Carbon Chemistry and Ocean Acidifi cation
The marine carbonate buff er system allows the ocean to take up CO
2
far in excess of its potential uptake capacity based on solubil-
ity alone, and in doing so controls the pH of the ocean. This control is achieved by a series of reactions that transform carbon added
as CO
2
into HCO
3
–
and CO
3
2–
. These three dissolved forms (collectively known as DIC) are found in the approximate ratio CO
2
:HCO
3
–
:
CO
3
2–
of 1:100:10 (Equation (7.1)). CO
2
is a weak acid and when it dissolves, it reacts with water to form carbonic acid, which dissociates
into a hydrogen ion (H
+
) and a HCO
3
–
ion, with some of the H
+
then reacting with CO
3
2–
to form a second HCO
3
–
ion (Equation (7.2)).
CO
2
+ H
2
O
→
H
+
+ HCO
3
–
→
2H
+
+ CO
3
2–
(7.1)
CO
2
+ H
2
O + CO
3
2–
→
HCO
3
–
+ H
+
+ CO
3
2–
→
2HCO
3
–
(7.2)
Therefore, the net result of adding CO
2
to seawater is an increase in H
+
and HCO
3
–
, but a reduction in CO
3
2–
. The decrease in the
CO
3
2–
ion reduces the overall buff ering capacity as CO
2
increases, with the result that proportionally more H
+
ions remain in solution
and increase acidity.
This ocean acidifi cation is leading to a decrease in the saturation state of CaCO
3
in the ocean. Two primary eff ects are expected:
(1) the biological production of corals as well as calcifying phytoplankton and zooplankton within the water column may be inhibited
or slowed down (Royal Society, 2005), and (2) the dissolution of CaCO
3
at the ocean fl oor will be enhanced (Archer, 2005). Aragonite,
the meta-stable form of CaCO
3
produced by corals and pteropods (planktonic snails; Lalli and Gilmer, 1989), will be particularly sus-
ceptible to a pH reduction (Kleypas et al., 1999b; Hughes et al., 2003; Orr et al., 2005).
Laboratory experiments under high ambient CO
2
with the coccolithophore species
Emiliania huxleyi
and
Gephyrocapsa oceanica
produce a signifi cant reduction in CaCO
3
production
and a stimulation of POC production (Riebesell et al., 2000; Zondervan et al., 2001). Other species and growth under other conditions
may show diff erent responses, so that no conclusive quantifi cation of the CaCO
3
feedback is possible at present (Tortell et al., 2002;
Sciandra et al., 2003).
The sinking speed of marine particle aggregates depends on their composition: CaCO
3
may act as an effi
cient ballast component,
leading to high sinking speeds of aggregates (Armstrong et al., 2002; Klaas and Archer, 2002). The relatively small negative feedback of
reduced CaCO
3
production to atmospheric pCO
2
may be compensated for by a change in the ballast for settling biogenic particles and
the associated shallowing of re-mineralization depth levels in the water column for organic carbon (Heinze, 2004). On the other hand,
production of extracellular organic carbon could increase under high CO
2
levels and lead to an increase in export (Engel et al., 2004).
Ecological changes due to expected ocean acidifi cation may be severe for corals in tropical and cold waters (Gattuso et al., 1999;
Kleypas et al., 1999a; Langdon et al., 2003; Buddemeier et al., 2004; Roberts et al., 2006) and for pelagic ecosystems (Tortell et al.,
2002; Royal Society, 2005). Acidifi cation can infl uence the marine food web at higher trophic levels (Langenbuch and Pörtner, 2003;
Ishimatsu et al., 2004).
Since the beginning of the industrial revolution, sea surface pH has dropped by about 0.1 pH units (corresponding to a 30% in-
crease in the H ion concentration). The expected continued decrease may lead within a few centuries to an ocean pH estimated to have
occurred most recently a few hundred million years before present (Caldeira and Wickett, 2003; Key et al., 2004; Box 7.3, Figure 1).
According to a model experiment based on the IPCC Scenarios 1992a (IS92a) emission scenario, bio-calcifi cation will be reduced
by 2100, in particular within the Southern Ocean (Orr et al., 2005), and by 2050 for aragonite-producing organisms (see also Figure
10.24). It is important to note that ocean acidifi cation is not a direct consequence of climate change but a consequence of fossil fuel
CO
2
emissions, which are the main driver of the anticipated climate change.
Box 7.3, Figure 1.
(a) Atmospheric CO
2
emissions,
historical atmospheric CO
2
levels and predicted CO
2
concentrations from the given emission time series,
together with changes in ocean pH based on horizontally
averaged chemistry. The emission time series is based on
the mid-range IS92a emission scenario (solid line) prior to
2100 and then assumes that emissions continue until fos-
sil fuel reserves decline.
(b) Estimated maximum change
in surface ocean pH as a function of fi nal atmospheric
CO
2
pressure, and the transition time over which this
CO
2
pressure is linearly approached from 280 ppm. A:
Glacial-interglacial CO
2
changes; B: slow changes over
the past 300 Myr; C: historical changes in ocean surface
waters; D: unabated fossil fuel burning over the next few
centuries.
Source: Caldeira and Wickett (2003). Reprinted
with permission from Macmillan Publishers Ltd: Nature,
Caldeira and Wickett (2003), copyright (2003).
530
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
A t m o s p h e r e
Biological Pumps
Solution Pump
Organic Carbon Pump
CaCO
3
Counter Pump
Air
Surface
Ocean
Intermediate
Water
Deep
Ocean
Sediment
Cold
Fresh
Warm
Haline
Solubility
High
Low
Photosynthesis
Carbon
Consumption
Remineralization
Carbon
Release
Calcium Carbonate
Re-dissolution
Alkalinity
Release
Production of
Calcareous Shells
Alkalinity
Consumption
POC flux
CaCO
3
flux
U
P
W
E
L
L
I
N
G
U
P
W
E
L
L
I
N
G
CO
2
CO
2
CO
2
CO
2
CO
2
CO
2
Figure 7.10.
Three main ocean carbon pumps govern the regulation of natural atmospheric CO
2
changes by the ocean (Heinze et al., 1991): the solubility pump, the organic
carbon pump and the CaCO
3
‘counter pump’. The oceanic uptake of anthropogenic CO
2
is dominated by inorganic carbon uptake at the ocean surface and physical transport of
anthropogenic carbon from the surface to deeper layers. For a constant ocean circulation, to fi rst order, the biological carbon pumps remain unaffected because nutrient cycling
does not change. If the ocean circulation slows down, anthropogenic carbon uptake is dominated by inorganic buffering and physical transport as before, but the marine particle
fl ux can reach greater depths if its sinking speed does not change, leading to a biologically induced negative feedback that is expected to be smaller than the positive feedback
associated with a slower physical downward mixing of anthropogenic carbon. Reprinted with permission, copyright 1991 American Geophysical Union.
the release of CO
2
in surface waters during formation of CaCO
3
shell material by plankton (‘CaCO
3
counter pump’).
Organic particles are re-mineralized (oxidized to DIC and
other inorganic compounds through the action of bacteria)
primarily in the upper 1,000 m of the oceanic water column,
with an accompanying decrease in dissolved O. On the average,
CaCO
3
particles sink deeper before they undergo dissolution:
deep waters are undersaturated with respect to CaCO
3
. The
remainder of the particle
fl
ux enters marine sediments and
is subject to either re-dissolution within the water column or
accumulation within the sediments. Although the POC reservoir
is small, it plays an important role in keeping DIC concentrations
low in surface waters and high in deep waters. The loop is closed
through the three-dimensional ocean circulation: upwelling
water brings inorganic carbon and nutrients to the surface
again, leading to outgassing and biogenic particle production.
Dissolved organic carbon enters the ocean water column from
rivers and marine metabolic processes. A large fraction of
DOC has a long ocean residence time (1–10 kyr), while other
fractions are more short-lived (days to hundreds of years; Loh
et al., 2004). The composition of dissolved organic matter is
still largely unknown.
In conjunction with the global ocean mixing or overturning
time of the order of 1 kyr (Broecker and Peng, 1982), small
changes in the large ocean carbon reservoir can induce
signi
fi
cant changes in atmospheric CO
2
concentration.
Likewise, perturbations in the atmospheric pCO
2
can be
buffered by the ocean. Glacial-interglacial changes in the
atmospheric CO
2
content can potentially be attributed to a
change in functioning of the marine carbon pump (see Chapter
6). The key role for the timing of the anthropogenic carbon
uptake by the ocean is played by the downward transport of
surface water, with a high burden of anthropogenic carbon,
into the ocean’s interior. The organic carbon cycle and the
CaCO
3
counter pump modulate, but do not dominate, the net
marine uptake of anthropogenic carbon.
531
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.3.4.2
Carbon Cycle Feedbacks to Changes in
Atmospheric Carbon Dioxide
Chemical buffering of anthropogenic CO
2
is the
quantitatively most important oceanic process acting as a
carbon sink. Carbon dioxide entering the ocean is buffered due
to scavenging by the CO
3
2–
ions and conversion to HCO
3
–
, that
is, the resulting increase in gaseous seawater CO
2
concentration
is smaller than the amount of CO
2
added per unit of seawater
volume. Carbon dioxide buffering in seawater is quanti
fi
ed by
the Revelle factor (‘buffer factor’, Equation (7.3)), relating the
fractional change in seawater pCO
2
to the fractional change in
total DIC after re-equilibration (Revelle and Suess, 1957; Zeebe
and Wolf-Gladrow, 2001):
Revelle factor (or buffer factor)
=
(
Δ
[CO
2
] / [CO
2
]) / (
Δ
[DIC] / [DIC])
(7.3)
The lower the Revelle factor, the larger the buffer capacity
of seawater. Variability of the buffer factor in the ocean depends
mainly on changes in pCO
2
and the ratio of DIC to total alkalinity.
In the present-day ocean, the buffer factor varies between 8 and
13 (Sabine et al., 2004a; Figure 7.11). With respect to atmospheric
pCO
2
alone, the inorganic carbon system of the ocean reacts in two
ways: (1) seawater re-equilibrates, buffering a signi
fi
cant amount
of CO
2
from the atmosphere depending on the water volume
exposed to equilibration; and (2) the Revelle factor increases
with pCO
2
(positive feedback; Figure 7.11). Both processes are
quantitatively important. While the
fi
rst is generally considered
as a system response, the latter is a feedback process.
The ocean will become less alkaline (seawater pH will
decrease) due to CO
2
uptake from the atmosphere (see Box 7.3).
Figure 7.11.
(a) The Revelle factor (or buffer factor) as a function of CO
2
partial pressure (for temperature 25°C, salinity 35 psu, and total alkalinity 2,300 µmol kg
–1
)
(Zeebe and Wolf-Gladrow, 2001, page 73; reprinted with permission, copyright 2001 Elsevier). (b) The geographical distribution of the buffer factor in ocean surface waters
in 1994 (Sabine et al., 2004a; reprinted with permission, copyright 2004 American Association for the Advancement of Science). High values indicate a low buffer capacity
of the surface waters.
The ocean’s capacity to buffer increasing atmospheric CO
2
will
decline in the future as ocean surface pCO
2
increases (Figure
7.11a). This anticipated change is certain, with potentially
severe consequences.
Increased carbon storage in the deep ocean leads to the
dissolution of calcareous sediments below their saturation
depth (Broecker and Takahashi, 1978; Feely et al., 2004). The
feedback of CaCO
3
sediment dissolution to atmospheric pCO
2
increase is negative and quantitatively signi
fi
cant on a 1 to
100 kyr time scale, where CaCO
3
dissolution will account for
a 60 to 70% absorption of the anthropogenic CO
2
emissions,
while the ocean water column will account for 22 to 33% on
a time scale of 0.1 to 1 kyr. In addition, the remaining 7 to
8% may be compensated by long-term terrestrial weathering
cycles involving silicate carbonates (Archer et al., 1998).
Due to the slow CaCO
3
buffering mechanism (and the slow
silicate weathering), atmospheric pCO
2
will approach a new
equilibrium asymptotically only after several tens of thousands
of years (Archer, 2005; Figure 7.12).
Elevated ambient CO
2
levels appear to also in
fl
uence
the production rate of POC by marine calcifying planktonic
organisms (e.g., Zondervan et al., 2001). This increased carbon
fi
xation under higher CO
2
levels was also observed for three
diatom (siliceous phytoplankton) species (Riebesell et al.,
1993). It is critical to know whether these increased carbon
fi
xation rates translate into increased export production rates
(i.e., removal of carbon to greater depths). Studies of the nutrient
to carbon ratio in marine phytoplankton have not yet shown
any signi
fi
cant changes related to CO
2
concentration of the
nutrient utilisation ef
fi
ciency (expressed through the ‘Red
fi
eld
ratio’ – carbon:nitrogen:phosphorus:silicon) in organic tissue
(Burkhardt et al., 1999).
532
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.3.4.3
Carbon Cycle Feedbacks to Changes in Physical
Forcing
A more sluggish ocean circulation and increased density
strati
fi
cation, both expected in a warmer climate, would slow
down the vertical transport of carbon, alkalinity and nutrients,
and the replenishment of the ocean surface with water that has not
yet been in contact with anthropogenic CO
2
. This narrowing of
the ‘bottleneck’ for anthropogenic CO
2
invasion into the ocean
would provide a signi
fi
cant positive feedback to atmospheric
greenhouse gas concentrations (Bolin and Eriksson, 1959; see
also the carbon cycle climate model simulations by Cox et al.,
2000; Friedlingstein et al., 2001, 2006). As long as the vertical
transfer rates for marine biogenic particles remain unchanged,
in a more sluggish ocean the biological carbon pump will be
more ef
fi
cient (Boyle, 1988; Heinze et al., 1991), thus inducing
a negative feedback, which is expected to be smaller than the
physical transport feedback (Broecker, 1991; Maier-Reimer
et al., 1996; Plattner et al., 2001; see Figure 7.10). However,
a modelling study by Bopp et al. (2005) predicts a decrease
in vertical particle transfer and hence shallower depths of
re-mineralization of particulate organic carbon resulting in a
positive CO
2
feedback. Further changes in plankton community
structure including the role of N
2
-
fi
xing organisms can feed
back to the carbon cycle (Sarmiento et al., 2004; Mahaffey
et al., 2005). Changes in ocean circulation can affect the
regional circulation of shelf and coastal seas, leading either
to increased export of nutrients plus carbon from the shallow
seas into the open ocean or to increased upwelling of nutrients
plus carbon onto the shelf and towards coastal areas (Walsh,
1991; Smith and Hollibaugh, 1993; Chen et al., 2003; Borges,
2005). A reduction in sea ice cover may increase the uptake
area for anthropogenic CO
2
and act as a minor negative carbon
feedback (ACIA, 2005). The physical ‘bottleneck’ feedback
dominates over biological feedbacks induced by circulation
change, resulting in an anticipated overall positive feedback to
climate change. Both feedbacks depend on details of the future
ocean circulation and model projections show a large range.
The solubility of CO
2
gas in seawater and the two dissociation
constants of carbonic acid in seawater depend on temperature
and salinity (Weiss, 1974; Millero et al., 2002). A 1°C increase
in sea surface temperature produces an increase in pCO
2
of 6.9
to 10.2 ppm after 100 to 1,000 years (Heinze et al., 2003; see
also Broecker and Peng, 1986; Plattner et al., 2001). Warming
may increase the biological uptake rate of nutrients and carbon
from surface waters, but the net effect on export and DIC is
uncertain. Laws et al. (2000) proposed that export ef
fi
ciency
increases with net photosynthesis at low temperatures, which
implies a positive feedback to warming. In addition, DOC may
be degraded more quickly at higher temperatures.
7.3.4.4
Carbon Cycle Feedbacks Induced by Nutrient
Cycling and Land Ocean Coupling
Rivers deliver carbon (DIC, DOC) and nutrients to the
ocean. Rising CO
2
levels in the atmosphere and land use may
lead to increased chemical and physical weathering, resulting
in increased carbon and alkalinity loads in rivers (Clair et al.,
1999; Hejzlar et al., 2003; Raymond and Cole, 2003; Freeman
et al., 2004). Depending on the lithology and soil composition of
the catchment areas, increased levels of alkalinity, DIC or DOC
can lead to local positive or negative feedbacks. Mobilisation
of silicate carbonates from soils and transfer to the ocean would
lead to a negative feedback to atmospheric CO
2
on long time
scales (Dupre et al., 2003). Variations in nutrient supply can
lead to species shifts and to deviations from the large-scale
average Red
fi
eld ratios mainly in coastal waters, but also in the
open ocean (Pahlow and Riebesell, 2000). Nutrient supply to
the ocean has been changed through increased nitrate release
from land due to fertilizer use as well as nitrogen deposition
from the atmosphere in highly polluted areas (De Leeuw et al.,
2001; Green et al., 2004).
Dust deposition to the ocean provides an important source
of micronutrients (iron, zinc and others, e.g., Frew et al., 2001;
Boyd et al., 2004) and ballast material to the ocean. Areas
where iron is not supplied by aeolian dust transport in suf
fi
cient
amounts tend to be iron-limited. A warmer climate may result
on the average in a decrease of dust mobilisation and transport
(Werner et al., 2002; Mahowald and Luo, 2003) although
increased dust loads may result as well due to changes in land
Figure 7.12.
Model projections of the neutralization of anthropogenic CO
2
for an
ocean-only model, a model including dissolution of CaCO
3
sediment and a model
including weathering of silicate rocks, (top) for a total of 1,000 GtC of anthropogenic
CO
2
emissions and (bottom) for a total of 5,000 GtC of anthropogenic CO
2
. Note that
the y-axis is different for the two diagrams. Without CaCO
3
dissolution from the sea-
fl oor, the buffering of anthropogenic CO
2
is limited. Even after 100 kyr, the remaining
pCO
2
is substantially higher than the pre-industrial value. Source: Archer (2005).
533
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
use (Tegen et al., 2004) and in vegetation cover (Woodward
et al., 2005). A decrease in dust loads could result in a net
positive feedback, further increasing CO
2
through a weakening
of marine biological production and export of aggregates due
to clay ballast (Haake and Ittekkot, 1990; Ittekkot, 1993).
Changes in plankton species composition and regional shifts of
high production zones due to a changing climate could lead to
a series of further feedbacks. Light absorption due to changes
in bio-optical heating may change and induce a respective
temperature change in ocean surface water (Sathyendranath et
al., 1991; Wetzel et al., 2006). An increase in blooms involving
calcifying organisms as indicated for the high northern latitudes
(Broerse et al., 2003; Smyth et al., 2004) can temporarily
increase surface ocean albedo, though the effect on the radiation
budget is small (Tyrell et al., 1999).
7.3.4.5
Summary of Marine Carbon Cycle Climate
Couplings
Couplings between the marine carbon cycle and climate are
summarised in Table 7.3 and below.
7.3.4.5.1
Robust
fi
ndings
•
A potential slowing down of the ocean circulation
and the decrease of seawater buffering with rising
CO
2
concentration will suppress oceanic uptake of
anthropogenic CO
2
.
•
Ocean CO
2
uptake has lowered the average ocean pH
(increased acidity) by approximately 0.1 since 1750. Ocean
acidi
fi
cation will continue and is directly and inescapably
coupled to the uptake of anthropogenic CO
2
by the ocean.
•
Inorganic chemical buffering and dissolution of marine
CaCO
3
sediments are the main oceanic processes for
neutralizing anthropogenic CO
2
. These processes cannot
prevent a temporary buildup of a large atmospheric
CO
2
pool because of the slow large-scale overturning
circulation.
7.3.4.5.2
Key uncertainties
•
Future changes in ocean circulation and density
strati
fi
cation are still highly uncertain. Both the physical
uptake of CO
2
by the ocean and changes in the biological
cycling of carbon depend on these factors.
•
The overall reaction of marine biological carbon cycling
(including processes such as nutrient cycling as well
as ecosystem changes including the role of bacteria and
viruses) to a warm and high-CO
2
world is not yet well
understood. Several small feedback mechanisms may add
up to a signi
fi
cant one.
•
The response of marine biota to ocean acidi
fi
cation is not
yet clear, both for the physiology of individual organisms
and for ecosystem functioning as a whole. Potential impacts
are expected especially for organisms that build CaCO
3
shell material (‘bio-calci
fi
cation’). Extinction thresholds
will likely be crossed for some organisms in some regions
in the coming century.
7.3.5
Coupling Between the Carbon Cycle and
Climate
7.3.5.1 Introduction
Atmospheric CO
2
is increasing at only about half the rate
implied by fossil fuel plus land use emissions, with the remainder
being taken up by the ocean, and vegetation and soil on land.
Therefore, the land and ocean carbon cycles are currently
helping to mitigate CO
2
-induced climate change. However,
these carbon cycle processes are also sensitive to climate. The
glacial-interglacial cycles are an example of tight coupling
between climate and the carbon cycle over long time scales,
but there is also clear evidence of the carbon cycle responding
to short-term climatic anomalies such as the El Niño-Southern
Oscillation (ENSO) and Arctic Oscillation (Rayner et al., 1999;
Bousquet et al., 2000; C. Jones et al., 2001; Lintner, 2002;
Russell and Wallace, 2004) and the climate perturbation arising
from the Mt. Pinatubo volcanic eruption (Jones and Cox, 2001a;
Lucht et al., 2002; Angert et al., 2004).
Previous IPCC reports have used simpli
fi
ed or ‘reduced-
form’ models to estimate the impact of climate change on the
carbon cycle. However, detailed climate projections carried
out with Atmosphere-Ocean General Circulation Models
(AOGCMs) have typically used a prescribed CO
2
concentration
scenario, neglecting two-way coupling between climate and
the carbon cycle. This section discusses the
fi
rst generation of
coupled climate-carbon cycle AOGCM simulations, using the
results to highlight a number of critical issues in the interaction
between climate change and the carbon cycle.
7.3.5.2
Coupled Climate-Carbon Cycle Projections
The TAR reported two initial climate projections using
AOGCMs with interactive carbon cycles. Both indicated
positive feedback due largely to the impacts of climate warming
on land carbon storage (Cox et al., 2000; Friedlingstein et al.,
2001), but the magnitude of the feedback varied markedly
between the models (Friedlingstein et al., 2003). Since the
TAR a number of other climate modelling groups have
completed climate-carbon cycle projections (Brovkin et al.,
2004; Thompson et al., 2004; N. Zeng et al., 2004, Fung et al.,
2005; Kawamiya et al., 2005; Matthews et al., 2005; Sitch et
al., 2005) as part of C
4
MIP. The 11 models involved in C
4
MIP
differ in the complexity of their components (Friedlingstein et
al., 2006), including both Earth System Models of Intermediate
Complexity and AOGCMs.
The models were forced by historical and Special Report
on Emission Scenarios (SRES; IPCC, 2000) A2 anthropogenic
CO
2
emissions for the 1850 to 2100 time period. Each modelling
group carried out at least two simulations: one ‘coupled’ in which
climate change affects the carbon cycle, and one ‘uncoupled’
in which atmospheric CO
2
increases do not in
fl
uence climate
(so that the carbon cycle experiences no CO
2
-induced climate
change). A comparison of the runs de
fi
nes the climate-
carbon cycle feedback, quanti
fi
ed by the feedback factor:
534
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
T
able 7.3.
Couplings between c
lima
te change (increased a
tmospheric pCO
2
, warming) and ocean carbon c
yc
le processes.
The response in terms of direct radia
tive forcing is considered (furthering or cou
nteracting uptake of
anthropogenic CO
2
from the a
tmosphere).
The two quantita
tively most important marine processes for neutraliza
tion of anthropogenic CO
2
work on long time scales only and are virtually certain to be in effect.
Marine Carbon Cycle
Pr
ocess
Major For
cing Factors
Response
+ = positive feedback
– = negative feedback
and
Quantitative Potential
Start
Re-equilibration
Time Scale (kyr)
Likelihood
Comment
Biological export
pr
oduction of or
ganic
carbon and changes in
or
ganic carbon cycling
W
arming, ocean cir
culation,
nutrient supply
, radiation,
atmospheric CO
2
, pH value
(Sum of ef
fects not clear)
+/–
medium
immediate
0.001–10
Likely
Complex feedback chain,
reactions can be fast for
surface ocean, nutrient
supply fr
om land works
on longer time scales,
patter
ns of biodiversity and
ecosystem functioning may
be af
fected
Biological export
pr
oduction of calcium
carbonate
W
arming, atmospheric CO
2
,
pH value
(Sum of ef
fects not clear)
+/–
small
immediate
0.001–1
Likely
Complex feedback chain,
extinction of species likely
,
patter
ns of biodiversity and
ecosystem functioning may
be af
fected
Seawater buf
fering
Atmospheric CO
2
, ocean
cir
culation
–
high
immediate
5–10
V
irtually certain
System r
esponse, leads to
ocean acidifi
cation
Changes in inor
ganic
carbon chemistry
(solubility
, dissociation,
buf
fer factor)
W
arming, atmospheric CO
2
,
ocean cir
culation
+
medium
immediate
5–10
V
irtually certain
Positive feedback
dependent on ‘bottleneck’
ocean mixing
Dissolution of calcium
carbonate sediments
pH value, ocean cir
culation
–
high
immediate
40
V
irtually certain
Patter
ns of biodiversity and
ecosystem functioning in
deep sea may be af
fected
W
eathering of silicate
carbonates
Atmospheric CO
2
, warming
–
medium
immediate
100
Likely
V
e
ry long-term negative
feedback
535
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
F
=
Δ
C
A
c
/
Δ
C
A
u
,where
Δ
C
A
c
is the change in CO
2
in the coupled
run, and
Δ
C
A
u
is the change in CO
2
in the uncoupled run. All
of the eleven C
4
MIP models produce a positive climate-carbon
cycle feedback, but with feedback factors varying from 1.04
(Model E) to 1.44 (Model A). This translates into an additional
CO
2
concentration of between 20 and 224 ppm by 2100, with a
mean of 87 ppm (Table 7.4).
All C
4
MIP models predict that an increasing fraction of total
anthropogenic CO
2
emissions will remain airborne through
the 21st century. Figure 7.13 shows the simulated partitioning
of anthropogenic CO
2
for the entire simulation period to 2100
from each of the coupled models, and compares this with the
partitioning simulated by the same models over the historical
period to 1999. The dashed box shows observational constraints
on the historical CO
2
partitioning, based on estimates of
changes in ocean carbon storage (Sabine et al., 2004a) and total
anthropogenic CO
2
emissions. The area of this box is largely due
to uncertainties in the net land use emissions. The majority of the
models sit within or very close to the historical constraints, but
they differ in the magnitude of the changes projected for the 21st
century. However, all models produce an increase in the fraction
of total emissions that remain in the atmosphere, and most also
indicate a decline in the fraction of emissions absorbed by the
ocean (9 out of 11 models) and the land (10 out of 11 models).
In the case of the oceanic uptake, this is largely a consequence of
the reduced buffering capacity as CO
2
increases, and therefore
also occurs in the uncoupled C
4
MIP models.
7.3.5.3 Sensitivity
Analysis
The coupled and uncoupled model experiments can be used
to separate the effects of climate change and CO
2
increase on
land and ocean carbon storage (Friedlingstein et al., 2003). Table
7.4 also shows the linear sensitivity parameters diagnosed from
each of the C
4
MIP models (Friedlingstein et al., 2006).
7.3.5.3.1 Increase in ocean carbon uptake with increasing
atmospheric carbon dioxide
The ocean takes up CO
2
at a rate that depends on the
difference between pCO
2
in the atmosphere and in the surface
ocean. Model estimates of uptake differ primarily because of
differences in the rate at which carbon is exported from the
surface ocean to depth by the large-scale circulation (Doney
et al., 2004; Section 7.3.4.1; Box 7.3) and the biological
pump (Sarmiento et al., 2004). Ocean carbon cycle model
intercomparisons have shown that the simulated circulation in
the Southern Ocean can have a large impact on the ef
fi
ciency
with which CO
2
, and other anthropogenic tracers such as CFCs,
Table 7.4.
Impact of carbon cycle feedbacks in the C
4
MIP models. Column 2 shows the impact of climate change on the CO
2
concentration by 2100, and column 3 shows the
related amplifi cation of the atmospheric CO
2
increase (i.e., the climate-carbon cycle feedback factor). Columns 4 to 8 list effective sensitivity parameters of the models:
transient sen-
sitivity of mean global temperature to CO
2
, and the sensitivities of land and ocean carbon storage to CO
2
and climate (Friedlingstein et al., 2006). These parameters were calculated
by comparison of the coupled and uncoupled runs over the entire period of the simulations (typically 1860 to 2100). Model details are given in Friedlingstein et al. (2006).
Model
a
Impact of
Climate
Change on
the CO
2
Concentration
by 2100 (ppm)
Climate-
Carbon
Feedback
Factor
Transient
Climate
Sensitivity
to Doubling
CO
2
(°C)
Land Carbon
Storage
Sensitivity
to CO
2
(GtC
ppm
–1
)
Ocean
Carbon
Storage
Sensitivity
to CO
2
(GtC
ppm
–1
)
Land
Carbon
Storage
Sensitivity
to Climate
(GtC °C
–1
)
Ocean Carbon
Storage
Sensitivity to
Climate (GtC
°C
–1
)
A. HadCM3LC
224
1.44
2.3
1.3
0.9
–175
–24
B. IPSL-CM2C
74
1.18
2.3
1.6
1.6
–97
–30
C. MPI-M
83
1.18
2.6
1.4
1.1
–64
–22
D. LLNL
51
1.13
2.5
2.5
0.9
–81
–14
E. NCAR CSM-1
20
1.04
1.2
1.1
0.9
–24
–17
F. FRCGC
128
1.26
2.3
1.4
1.2
–111
–47
G. Uvic-2.7
129
1.25
2.3
1.2
1.1
–97
–43
H. UMD
98
1.17
2.0
0.2
1.5
–36
–60
I. BERN-CC
65
1.15
1.5
1.6
1.3
–104
–38
J. CLIMBER2-LPJ
59
1.11
1.9
1.2
0.9
–64
–22
K. IPSL-CM4-LOOP
32
1.07
2.7
1.2
1.1
–19
–17
Mean
87
1.18
2.1
1.4
1.1
–79
–30
Standard Deviation
±57
±0.11
±0.4
±0.5
±0.3
±45
±15
Notes:
a
HadCM3LC: Hadley Centre coupled climate-carbon cycle general circulation model; IPSL-CM2C: Institut Pierre-Simon Laplace; MPI-M: Max Planck Institute for Meteorology;
LLNL: Lawrence Livermore National Laboratory; NCAR CSM-1: NCAR Climate System Model version 1; FRCGC: Frontier Research Center for Global Change; Uvic-2.7:
University of Victoria Earth System Climate Model; UMD: University of Maryland; BERN-CC: Bern Carbon Cycle Model; CLIMBER2-LPJ: Climate Biosphere Model 2 - Lund
Potsdam Jena Terrestrial Carbon Model; IPSL-CM4-LOOP: Institute Pierre-Simon Laplace.
536
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
are drawn down (Orr et al., 2001; Dutay et al., 2002). The
C
4
MIP models show ocean carbon storage increases ranging
from 0.9 to 1.6 GtC ppm
–1
, which is equivalent to ocean uptake
increasing at between 42 and 75% of the rate of atmospheric
CO
2
increase. Basic ocean carbonate chemistry suggests that
the ocean-borne fraction of emissions will fall in the future,
even in the absence of climate change, because of an increasing
ocean buffer factor (Section 7.3.4.2).
7.3.5.3.2
Increase in land carbon uptake with increasing
atmospheric carbon dioxide
In the absence of land use change and forest
fi
res, land carbon
storage depends on the balance between the input of carbon as
NPP, and the loss of carbon as heterotrophic (soil) respiration
(Section 7.3.3). There is an ongoing debate concerning the
importance of CO
2
fertilization at the patch scale where other
constraints such as N limitation may dominate; recent surveys
indicate a wide range of possible responses to a CO
2
increase of
around 50%, with average increases of 12 to 23% (Norby et al.,
2005; see Section 7.3.3.1).
The C
4
MIP models show increases in global NPP of
between 6 and 33% when CO
2
increases over the same range.
These
fi
gures are not directly comparable: some C
4
MIP models
include vegetation dynamics, which are likely to increase the
vegetation cover as well as the NPP per unit of vegetation
area, and therefore lead to higher overall sensitivity of global
NPP to CO
2
. The FACE experiments also typically involve an
instantaneous increase in CO
2
. However, most C
4
MIP models
are within the range of the CO
2
sensitivities measured.
The overall response of land carbon storage to CO
2
is given
by the
fi
fth column of Table 7.4. The C
4
MIP models show
time-mean land carbon storage increases ranging from 0.2 to
2.5 GtC ppm
–1
, with all but two models between 1.1 and 1.6
GtC ppm
–1
. This response is driven by the CO
2
fertilization of
NPP in each model, with a counteracting tendency for the mean
soil carbon turnover rate (i.e., the heterotrophic respiration by
unit soil carbon) to increase even in the absence of climate
change. This somewhat surprising effect of CO
2
is seen to
varying degrees in all C
4
MIP models. It appears to arise because
CO
2
fertilization of NPP acts particularly to increase vegetation
carbon, and therefore litter fall and soil carbon, in productive
tropical regions that have high intrinsic decomposition rates.
This increases the average turnover rate of the global soil carbon
pool even though local turnover rates are unchanged. In some
models (e.g., model C) this acts to offset a signi
fi
cant fraction
of the land carbon increase arising from CO
2
fertilization.
Models with large responses of ocean or land carbon storage
to CO
2
tend to have weaker climate-carbon cycle feedbacks
because a signi
fi
cant fraction of any carbon released through
climate change effects is reabsorbed through direct CO
2
effects
(Thompson et al., 2004).
7.3.5.3.3
Transient climate sensitivity to carbon dioxide
The strength of the climate-carbon cycle feedback loop
depends on both the sensitivity of the carbon cycle to climate,
and the sensitivity of climate to CO
2
. The equilibrium climate
sensitivity to a doubling of atmospheric CO
2
concentration
remains a critical uncertainty in projections of future climate
change, but also has a signi
fi
cant bearing on future CO
2
concentrations, with higher climate sensitivities leading to
larger climate-carbon cycle feedbacks (Andreae et al., 2005).
The fourth column of Table 7.4 shows the transient global
climate sensitivity (i.e., the global climate warming that results
when the transient simulation passes doubled atmospheric CO
2
)
for each of the C
4
MIP models. All but two models (models E
and I) have transient climate sensitivities in the range 1.9°C
to 2.7°C. However, differences in carbon cycle responses
are likely to occur because of potentially large differences in
regional climate change, especially where this affects water
availability on the land.
7.3.5.3.4
Dependence of ocean carbon uptake on climate.
Climate change can reduce ocean uptake through reductions
in CO
2
solubility, suppression of vertical mixing by thermal
strati
fi
cation and decreases in surface salinity. On longer time
scales (>70 years) the ocean carbon sink may also be affected
by climate-driven changes in large-scale circulation (e.g.,
a slowing down of the thermohaline circulation). The last
column of Table 7.4 shows the sensitivity of ocean carbon
storage to climate change as diagnosed from the C
4
MIP models.
All models indicate a reduction in the ocean carbon sink by
climate change of between –14 and –60 GtC °C
–1
, implying a
positive climate-CO
2
feedback.
Figure 7.13.
Predicted increase in the fraction of total emissions that add to
atmospheric CO
2
. Changes in the mean partitioning of emissions as simulated by
the C
4
MIP models up to 2000 (black symbols) and for the entire simulation period to
2100 (red symbols). The letters represent the models as given in Table 7.4. The box
shown by the dotted line is a constraint on the historical carbon balance based on
records of atmospheric CO
2
increase, and estimates of total emissions (fossil fuel
plus land use emissions) and the oceanic uptake of anthropogenic CO
2
(Sabine et al.,
2004a). The black and red diamonds show the model-mean carbon partitioning for
the historical period and the entire simulation period, respectively. The red line shows
the mean tendency towards an increasing airborne fraction through the 21st century,
which is common to all models.
537
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.3.5.3.5
Dependence of land carbon storage on climate.
The major land-atmosphere
fl
uxes of CO
2
are strongly
climate dependent. Heterotrophic respiration and NPP are both
very sensitive to water availability and ambient temperatures.
Changes in water availability depend critically on uncertain
regional aspects of climate change projections and are therefore
likely to remain a dominant source of uncertainty (see Chapter
11). The overall sensitivity of land carbon storage to climate
(Table 7.4, seventh column) is negative in all models, implying
a positive climate-CO
2
feedback, but the range is large: –19 to
–175 GtC °C
–1
. These values are determined by the combined
effects of climate change on NPP and the soil carbon turnover
(or decomposition) rate, as shown in Table 7.5.
The C
4
MIP models utilise different representations of soil
carbon turnover, ranging from single-pool models (model A) to
nine-pool models (model E). However, most soil models assume
a similar acceleration of decay with temperature, approximately
equivalent to a doubling of the speci
fi
c respiration rate for
every 10°C warming. This temperature sensitivity is broadly
consistent with a long history of lab and
fi
eld measurements of
soil ef
fl
ux (Raich and Schlesinger, 1992), although there is an
ongoing dif
fi
culty in separating root and soil respiration. Note,
however, that the expected dependence on temperature was not
found at the whole ecosystem level for decadal time scales, in
forest soils (Giardina and Ryan, 2000; Melillo et al., 2002),
grasslands (Luo et al., 2001) or boreal forests (Dunn et al., 2007).
These apparent discrepancies may re
fl
ect the rapid depletion
of labile pools of organic matter, with strong temperature
responses likely so long as litter inputs are maintained (Knorr
et al., 2005). Nevertheless, the temperature sensitivity of the
slow carbon pools is still poorly known.
Table 7.5 shows that all C
4
MIP models simulate an overall
increase in soil carbon turnover rate as the climate warms,
ranging from 2 to 10% per °C. The use of a single soil carbon
pool in the Hadley model (A) cannot completely account for
the relatively large sensitivity of soil respiration to temperature
in this model (Jones et al., 2005), as evidenced by the lower
effective sensitivity diagnosed from the UVic model (model G),
which uses the same soil-vegetation component. It seems more
likely that differences in soil moisture simulations are playing the
key part in determining the effective sensitivity of soil turnover
rate to climate. Table 7.5 also shows the effective sensitivities
of NPP to climate, ranging from a signi
fi
cant reduction of 6%
per °C to smaller climate-change driven increases of 2% per
°C under climate change. This variation may re
fl
ect different
time scales for boreal forest response to warming (leading to
a positive impact on global NPP), as well as different regional
patterns of climate change (Fung et al., 2005). The models with
the largest negative responses of NPP to climate (models A, B
and C) also show the tendency for tropical regions to dry under
climate change, in some cases signi
fi
cantly (Cox et al., 2004).
7.3.5.4
Summary of Coupling Between the Carbon Cycle
and Climate
7.3.5.4.1 Robust
fi
ndings
Results from the coupled climate-carbon cycle models
participating in the C
4
MIP project support the following
statements:
Table 7.5.
Effective sensitivities of land processes in the C
4
MIP models: percent change of vegetation NPP to a doubling of atmospheric CO
2
concentration (Column 2), and
sensitivities of vegetation NPP and specifi c heterotrophic soil respiration to a 1°C global temperature increase (Columns 3 and 4).
Model
a
Sensitivity of Vegetation NPP to CO
2
:
% change for a CO
2
doubling
Sensitivity of Vegetation NPP
to Climate:
% change for a 1°C increase
Sensitivity of Specifi c Heterotrophic
Respiration Rate to Climate:
% change for a 1°C increase
A. HadCM3LC
57
–5.8
10.2
B. IPSL-CM2C
50
–4.5
2.3
C. MPI-M
76
–4.0
2.8
D. LLNL
73
–0.4
7.0
E. NCAR CSM-1
34
0.8
6.2
F. FRCGC
21
1.2
7.2
G. UVic-2.7
47
–2.3
6.5
H. UMC
12
–1.6
4.8
I. BERN-CC
46
1.2
8.7
J. CLIMBER2-LPJ
44
1.9
9.4
K. IPSL-CM4-LOOP
64
–0.3
2.9
Mean
48
–1.3
6.2
Std Dev
±20
±2.6
±2.7
Notes:
a
See Table 7.4 for model descriptions.
538
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Figure 7.14.
Uncertainties in carbon cycle feedbacks estimated from analysis of the results from the C
4
MIP models. Each effect is given in terms of its impact on the mean
airborne fraction over the simulation period (typically 1860 to 2100), with bars showing the uncertainty range based on the ranges of effective sensitivity parameters given in
Tables 7.4 and 7.5. The lower three bars are the direct response to increasing atmospheric CO
2
(see Section 7.3.5 for details), the middle four bars show the impacts of climate
change on the carbon cycle, and the top black bar shows the range of climate-carbon cycle feedbacks given by the C
4
MIP models.
•
All C
4
MIP models project an increase in the airborne
fraction of total anthropogenic CO
2
emissions through the
21st century.
•
The CO
2
increase alone will lead to continued uptake by the
land and the ocean, although the ef
fi
ciency of this uptake
will decrease through the carbonate buffering mechanism in
the ocean, and through saturation of the land carbon sink.
•
Climate change alone will tend to suppress both land
and ocean carbon uptake, increasing the fraction of
anthropogenic CO
2
emissions that remain airborne and
producing a positive feedback to climate change. The
magnitude of this feedback varies among the C
4
MIP
models, ranging from a 4 to 44% increase in the rate of
increase of CO
2
, with a mean (± standard deviation) of 18 ±
11%.
7.3.5.4.2 Key
uncertainties
The C
4
MIP models also exhibit uncertainties in the
evolution of atmospheric CO
2
for a given anthropogenic
emissions scenario. Figure 7.14 shows how uncertainties in
the sensitivities of ocean and land carbon processes contribute
to uncertainties in the fraction of emissions that remain in the
atmosphere. The con
fi
dence limits were produced by spanning
the range of sensitivities diagnosed from the 11 C
4
MIP models
(Tables 7.4 and 7.5). In the absence of climate change effects
(lowest three bars), models simulate increased uptake by ocean
and land (primarily as a result of CO
2
enhancement of NPP),
with a slight offset of the land uptake by enhancement of the
speci
fi
c heterotrophic respiration rate (see Section 7.3.5.3.2).
However, there is a wide range of response to CO
2
, even in the
absence of climate change effects on the carbon cycle. Climate
change increases the fraction of emissions that remain airborne
by suppressing ocean uptake, enhancing soil respiration and
reducing plant NPP. The sensitivity of NPP to climate change
is especially uncertain because it depends on changing soil
water availability, which varies signi
fi
cantly between General
Circulation Models (GCMs), with some models suggesting
major drying and reduced productivity in tropical ecosystems
(Cox et al., 2004). The transient climate sensitivity to CO
2
is
also a major contributor to the overall uncertainty in the climate-
carbon cycle feedback (top bar).
Other potentially important climate-carbon cycle interactions
were not included in these
fi
rst generation C
4
MIP experiments.
The ocean ecosystem models used in C
4
MIP are at an early stage
of development. These models have simple representations of
the biological
fl
uxes, which include the fundamental response to
changes in internal nutrients, temperature and light availability,
but for most models do not include the more complex responses
539
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
to changes in ecosystem structure. Changes in ecosystem
structure can occur when speci
fi
c organisms respond to surface
warming, acidi
fi
cation, changes in nutrient ratios resulting
from changes in external sources of nutrients (atmosphere or
rivers) and changes in upper trophic levels (
fi
sheries). Shifts in
the structure of ocean ecosystems can in
fl
uence the rate of CO
2
uptake by the ocean (Bopp et al., 2005).
The
fi
rst-generation C
4
MIP models also currently exclude,
by design, the effects of forest
fi
res and prior land use change.
Forest regrowth may account for a large part of the land carbon
sink in some regions (e.g., Pacala et al., 2001; Schimel et al.,
2001; Hurtt et al., 2002; Sitch et al., 2005), while combustion
of vegetation and soil organic matter may be responsible for
a signi
fi
cant fraction of the interannual variability in CO
2
(Cochrane, 2003; Nepstad et al., 2004; Kasischke et al., 2005;
Randerson et al., 2005). Other important processes were
excluded in part because modelling these processes is even less
straightforward. Among these are N cycling on the land (which
could enhance or suppress CO
2
uptake by plants) and the
impacts of increasing ozone concentrations on plants (which
could suppress CO
2
uptake).
7.4
Reactive Gases and the Climate
System
The atmospheric concentration of many reactive gases has
increased substantially during the industrial era as a result
of human activities. Some of these compounds (CH
4
, N
2
O,
halocarbons, ozone, etc.) interact with longwave (infrared)
solar radiation and, as a result, contribute to ‘greenhouse
warming’. Ozone also ef
fi
ciently absorbs shortwave (ultraviolet
and visible) solar energy, so that it protects the biosphere
(including humans) from harmful radiation and plays a key
role in the energy budget of the middle atmosphere. Many
atmospheric chemical species are emitted at the surface as a
result of biological processes (soils, vegetation, oceans) or
anthropogenic activities (fossil fuel consumption, land use
changes) before being photochemically destroyed in the
atmosphere and converted to compounds that are eventually
removed by wet and dry deposition. The oxidizing power (or
capacity) of the atmosphere is determined primarily by the
atmospheric concentration of the OH radical (daytime) and to
a lesser extent the concentrations of the nitrate radical (NO
3
;
nighttime), ozone and hydrogen peroxide (H
2
O
2
). The coupling
between chemical processes in the atmosphere and the climate
system (Figure 7.15) are complex because they involve a large
number of physical, chemical and biological processes that
are not always very well quanti
fi
ed. An important issue is to
determine to what extent predicted climate change could affect
air quality (see Box 7.4). The goal of this section is assess recent
progress made in the understanding of the two-way interactions
between reactive gases and the climate system.
Figure 7.15.
Schematic representation of the multiple interactions between
tropospheric chemical processes, biogeochemical cycles and the climate system. RF
represents radiative forcing, UV ultraviolet radiation, T temperature and HNO
3
nitric acid.
7.4.1 Methane
7.4.1.1 Biogeochemistry and Budgets of Methane
Atmospheric CH
4
originates from both non-biogenic and
biogenic sources. Non-biogenic CH
4
includes emissions from
fossil fuel mining and burning (natural gas, petroleum and
coal), biomass burning, waste treatment and geological sources
(fossil CH
4
from natural gas seepage in sedimentary basins and
geothermal/volcanic CH
4
). However, emissions from biogenic
sources account for more than 70% of the global total. These
sources include wetlands, rice agriculture, livestock, land
fi
lls,
forests, oceans and termites. Emissions of CH
4
from most of these
sources involve ecosystem processes that result from complex
sequences of events beginning with primary fermentation of
organic macromolecules to acetic acid (CH
3
COOH), other
carboxylic acids, alcohols, CO
2
and hydrogen (H
2
), followed
by secondary fermentation of the alcohols and carboxylic acids
to acetate, H
2
and CO
2
, which are
fi
nally converted to CH
4
by
the so-called methanogenic Archaea: CH
3
COOH
→
CH
4
+ CO
2
and CO
2
+ 4H
2
→
CH
4
+ 2H
2
O (Conrad, 1996). Alternatively,
CH
4
sources can be divided into anthropogenic and natural.
The anthropogenic sources include rice agriculture, livestock,
land
fi
lls and waste treatment, some biomass burning, and fossil
fuel combustion. Natural CH
4
is emitted from sources such as
wetlands, oceans, forests,
fi
re, termites and geological sources
(Table 7.6).
540
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Box 7.4: Effects of Climate Change on Air Quality
Weather is a key variable aff ecting air quality. Surface air
concentrations of pollutants are highly sensitive to bound-
ary layer ventilation, winds, temperature, humidity and
precipitation. Anomalously hot and stagnant conditions in
the summer of 1988 were responsible for the highest ozone
year on record in the north-eastern USA (Lin et al., 2001). The
summer heat wave in Europe in 2003 was associated with
exceptionally high ozone (Ordonez et al., 2005). Such high
interannual variability of surface ozone correlated with tem-
perature demonstrates the potential air quality implications
of climate change over the next century.
A few GCM studies have investigated how air pollution
meteorology might respond to future climate change. Rind
et al. (2001) found that increased continental ventilation as
a result of more vigorous convection should decrease sur-
face concentrations, while Holzer and Boer (2001) found
that weaker winds should result in slower dilution of pol-
lution plumes and hence higher concentrations. A focused
study by Mickley et al. (2004) for the eastern USA found an
increase in the severity and persistence of regional pollution
episodes due to the reduced frequency of ventilation by cy-
clones tracking across Canada. This eff ect more than off sets
the dilution associated with the small rise in mixing depths. A decrease in cyclone frequency at northern mid-latitudes and a shift to
higher latitudes has been noted in observations from the past few decades (McCabe et al., 2001). An urban air quality model study
by Jacobson (1999) pointed out that decreasing soil moisture or increasing surface temperature would decrease mixing depths and
reduce near-surface pollutant concentrations.
A number of studies in the USA have shown that summer daytime ozone concentrations correlate strongly with temperature (NRC,
1991). This correlation appears to refl ect contributions of comparable magnitude from (1) temperature-dependent biogenic VOC
emissions, (2) thermal decomposition of peroxyacetylnitrate, which acts as a reservoir for NO
x
and (3) association of high temperatures
with regional stagnation (Jacob et al., 1993; Sillman and Samson, 1995; Hauglustaine et al., 2005). Empirical relationships between
ozone air quality standard exceedances and temperature, as shown in Figure 1, integrate all of these eff ects and could be used to
estimate how future regional changes in temperature would aff ect ozone air quality. Changes in the global ozone background would
also have to be accounted for (Stevenson et al., 2005).
A few GCM studies have examined more specifi cally the eff ect of changing climate on regional ozone air quality, assuming con-
stant emissions. Knowlton et al. (2004) use a GCM coupled to a Regional Climate Model (RCM) to investigate the impact of 2050 cli-
mate change (compared with 1990) on ozone concentrations in the New York City metropolitan area. They found a signifi cant ozone
increase that they translated into a 4.5% increase in ozone-related acute mortality. Langner et al. (2005) use an RCM driven by two
diff erent GCMs to examine changes in the Accumulated Ozone concentration above a Threshold of 40 ppb (AOT40) statistic (ozone-
hours above 40 ppb) over Europe in 2050 to 2070 relative to the present. They found an increase in southern and central Europe and
a decrease in northern Europe that they attributed to diff erent regional trends in cloudiness and precipitation. Dentener et al. (2006)
synthesise the results of 10 global model simulations for 2030 driven by future compared with present climate. They fi nd that climate
change caused mean decreases in surface ozone of 0.5 to 1 ppb over continents and 1 to 2 ppb over the oceans, although some con-
tinental regions such as the Eastern USA experienced slight increases.
There has been less work on the sensitivity of aerosols to meteorological conditions. Regional model simulations by Aw and Klee-
man (2003) fi nd that increasing temperatures should increase surface aerosol concentrations due to increased production of aerosol
precursors (in particular semi-volatile organic compounds and HNO
3
) although this is partly compensated by the increasing vapour
pressure of these compounds at higher temperatures. Perturbations of precipitation frequencies and patterns might be expected to
have a major impact on aerosol concentrations, but the GCM study by Mickley et al. (2004) for 2000 to 2050 climate change fi nds little
eff ect in the USA.
Box 7.4, Figure 1.
Probability that the daily maximum eight-hour average ozone
concentration will exceed the US National Ambient Air Quality Standard of 0.08 ppm
for a given daily maximum temperature based on 1980 to 1998 data. Values are
shown for New England (bounded by 36°N, 44°N, 67.5°W and 87.5°W), the Los An-
geles Basin (bounded by 32°N, 40°N, 112.5°W and 122.5°W) and the southeastern
USA (bounded by 32°N, 36°N, 72.5°W and 92.5°W). Redrawn from Lin et al. (2001).
541
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
The net rate of CH
4
emissions is generally estimated
from three approaches: (1) extrapolation from direct
fl
ux
measurements and observations, (2) process-based modelling
(bottom-up approach) and (3) inverse modelling that relies on
spatially distributed, temporally continuous observations of
concentration, and in some cases isotopic composition in the
atmosphere (top-down approach). The top-down method also
includes aircraft and satellite observations (Xiao et al., 2004;
Frankenberg et al., 2005, 2006). When the bottom-up approach
is used to extrapolate the emissions to larger scales, uncertainty
results from the inherent large temporal and spatial variations
of
fl
uxes and the limited range of observational conditions.
The top-down approach helps to overcome the weaknesses in
bottom-up methods. However, obstacles to extensive application
of the top-down approach include inadequate observations,
and insuf
fi
cient capabilities of the models to account for error
ampli
fi
cation in the inversion process and to simulate complex
topography and meteorology (Dentener et al., 2003a; Mikaloff
Fletcher et al., 2004a, 2004b; Chen and Prinn, 2005, 2006).
Measurements of isotopes of CH
4
(
13
C,
14
C, and
2
H) provide
additional constraints on CH
4
budgets and speci
fi
c sources,
but such data are even more limited (Bergamaschi et al., 2000;
Lassey et al., 2000; Mikaloff Fletcher et al., 2004a, 2004b).
Since the TAR, availability of new data from various
measurement networks and from national reporting documents
has enabled re-estimates of CH
4
source magnitudes and insights
into individual source strengths. Total global pre-industrial
emissions of CH
4
are estimated to be 200 to 250 Tg(CH
4
) yr
–1
(Chappellaz et al., 1993; Etheridge et al., 1998; Houweling
et al., 2000; Ferretti et al., 2005; Valdes et al., 2005). Of this,
natural CH
4
sources emitted between 190 and 220 Tg(CH
4
) yr
–1
,
and anthropogenic sources (rice agriculture, livestock, biomass
burning and waste) accounted for the rest (Houweling et al.,
2000; Ruddiman and Thomson, 2001). In contrast, anthropogenic
emissions dominate present-day CH
4
budgets, accounting for
more than 60% of the total global budget (Table 7.6).
The single largest CH
4
source is natural wetlands. Recent
estimates combine bottom-up and top-down
fl
uxes, and global
observations of atmospheric CH
4
concentrations in a three-
dimensional Atmospheric Transport and Chemical Model
(ATCM) simulation (Chen and Prinn, 2005, 2006). In these
estimates, southern and tropical regions account for more than
70% of total global wetland emissions. Other top-down studies
that include both direct observations and
13
C/
12
C ratios of CH
4
suggest greater emissions in tropical regions compared with
previously estimates (Mikaloff Fletcher et al., 2004a, 2004b;
Xiao et al., 2004; Frankenberg et al., 2006). However, several
bottom-up studies indicate fewer emissions from tropical rice
agriculture (Li et al., 2002; Yan et al., 2003; Khalil and Shearer
2006). Frankenberg et al. (2005, 2006) and Keppler et al.
(2006) suggest that tropical trees emit CH
4
via an unidenti
fi
ed
process. The
fi
rst estimate of this source was 10 to 30% (62–236
Tg(CH
4
) yr
–1
) of the global total, but Kirschbaum
et al. (2006)
revise this estimate downwards to 10 to 60 Tg(CH
4
) yr
–1
.
Representative
13
C/
12
C ratios (
δ
13
C values) of CH
4
emitted from
individual sources are included in Table 7.6. Due to isotope
fractionation associated with CH
4
production and consumption
processes, CH
4
emitted from each source exhibits a measurably
different
δ
13
C value. Therefore, it is possible, using mixing
models, to constrain further the sources of atmospheric CH
4
.
Geological sources of CH
4
are not included in Table 7.6.
However, several studies suggest that signi
fi
cant amounts of
CH
4
, produced within the Earth’s crust (mainly by bacterial
and thermogenic processes), are released into the atmosphere
through faults and fractured rocks, mud volcanoes on land and
the sea
fl
oor, submarine gas seepage, microseepage over dry
lands and geothermal seeps (Etiope and Klusman, 2002; Etiope,
2004; Kvenvolden and Rogers, 2005). Emissions from these
sources are estimated to be as large as 40 to 60 Tg(CH
4
) yr
–1
.
The major CH
4
sinks are oxidation by OH in the
troposphere, biological CH
4
oxidation in drier soil, and loss to
the stratosphere (Table 7.6). Oxidation by chlorine (Cl) atoms
in the marine atmospheric boundary layer is suggested as an
additional sink for CH
4
, possibly constituting an additional loss
of about 19 Tg(CH
4
) yr
–1
(Gupta et al., 1997; Tyler et al., 2000;
Platt et al., 2004; Allan et al., 2005). However, the decline in the
growth rate of atmospheric CH
4
concentration since the TAR
shows no clear correlation with change in sink strengths over
the same period (Prinn et al., 2001, 2005; Allan et al., 2005).
This trend has continued since 1993, and the reduction in the
CH
4
growth rate has been suggested to be a consequence of
source stabilisation and the approach of the global CH
4
budget
towards steady state (Dlugokencky et al., 1998, 2003). Thus,
total emissions are likely not increasing but partitioning
among the different sources may have changed (see Section
2.3). Consequently, in the Fourth Assessment Report (AR4)
the sink strength is treated as in the TAR (576 Tg(CH
4
) yr
–1
).
However, the AR4 estimate has been increased by 1% (to 581
Tg(CH
4
) yr
–1
) to take into account the recalibration of the CH
4
scale explained in Chapter 2. The main difference between TAR
and AR4 estimates is the source-sink imbalance inferred from the
annual increment in concentration. The TAR used 8 ppb yr
–1
for
a period centred on 1998 when there was clearly an anomalously
high growth rate. The present assessment uses 0.2 ppb yr
–1
, the
average over 2000 to 2005 (see Section 2.3 and Figure 2.4).
Thus, using the CH
4
growth rate for a single anomalous year, as
in the TAR, gives an anomalously high top-down value relative
to the longer-term average source. For a conversion factor of
2.78 Tg(CH
4
) per ppb and an atmospheric concentration
of 1,774 ppb, the atmospheric burden of CH
4
in 2005 was
4,932 Tg, with an annual average increase (2000–2005) of
about 0.6 Tg yr
–1
. Total average annual emissions during the
period considered here are approximately 582 Tg(CH
4
) yr
–1
.
Uncertainty in this estimate may arise from several sources.
Uncertainty in the atmospheric concentration measurement,
given in Chapter 2 as 1,774 ± 1.8 ppb in 2005, is small (about
0.1%). Uncertainty ranges for individual sink estimates are
±103 Tg(CH
4
) (20%), ±15 Tg(CH
4
) (50%), ±8 Tg(CH
4
) (20%)
for OH, soil and stratospheric loss, respectively (as reported in
the Second Assessment Report). The use of a different lifetime
for CH
4
(8.7 ± 1.3 years) leads to an uncertainty in overall sink
strength of ±15%. Thus, the top-down method used in AR4 is
542
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
T
able 7.6
Sources,
sinks and a
tmospheric budgets of CH
4
(Tg(CH
4
) yr
–1
).
a
Refer
ences
Indicative
13
C, ‰
b
Hein et al.,
1997
c
Houweling
et al.,
2000
c
Olivier et
al., 2005
W
uebbles and
Hayhoe, 2002
Scheehle et
al., 2002
J. W
ang
et al.,
2004
c
Mikalof
f
Fletcher et al.,
2004a
c
Chen and
Prinn, 2006
c
T
A
R
AR4
Base year
1983–1989
2000
1990
1994
1999
1996–2001
1998
2000–2004
Natural sour
ces
222
145
200
260
168
W
e
tlands
–58
231
163
100
176
231
145
T
ermites
–70
20
20
20
29
23
Ocean
–60
15
4
Hydrates
–60
5
4
Geological sour
ces
–40
4
1
4
Wild animals
–60
15
Wildfi
re
s
–25
5
2
Anthr
opogenic
sour
ces
361
320
358
264
307
350
428
Ener
gy
74
77
Coal mining
–37
32
34
46
30
48
d
Gas, oil, industry
–44
68
64
60
52
36
e
Landfi
lls & waste
–55
43
66
61
69
49
35
Ruminants
–60
92
80
81
76
83
91
189
f
Rice agricultur
e
–63
83
39
60
31
57
54
112
Biomass bur
ning
–25
43
50
14
41
88
43
e
C3 vegetation
–25
27
C4 vegetation
–12
9
T
otal sour
ces
592
503
507
610
596
598
582
Imbalance
+33
+22
+1
Sinks
Soils
–18
26
30
34
30
30
30
g
T
ropospheric OH
–3.9
488
445
428
507
506
511
g
Stratospheric loss
45
40
30
40
40
40
g
T
otal sink
559
515
492
577
576
581
g
Notes:
a
T
able shows the best estimate values.
b
Indicative
13
C values for sour
ces ar
e taken mainly fr
om Mikalof
f Fletcher et al. (2004a). Entries for sinks ar
e the fractionation, (k
13
/k
12
–1) wher
e k
n
is the r
emoval rate of
n
CH
4
; the fractionation for OH is taken fr
om
Sauer
essig et al. (2001) and that for the soil sink fr
om Snover and Quay (2000) as the most r
ecent determinations.
c
Estimates fr
om global inverse modelling (top-down method).
d
Includes natural gas emissions.
e
Biofuel emissions ar
e included under Industry
.
f
Includes emissions fr
om landfi
lls and wastes.
g
Numbers ar
e incr
eased by 1% fr
om the T
A
R accor
ding to r
ecalibration described in Chapter 2.
543
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
constrained mainly by uncertainty in sink estimates and the
choice of lifetime used in the mass balance calculation.
7.4.1.2
Effects of Climate
Effects of climate on CH
4
biogeochemistry are investigated
by examining records of the past and from model simulations
under various climate change scenarios. Ice core records going
back 650 ka (Petit et al., 1999; Spahni et al., 2005) reveal that the
atmospheric concentration of CH
4
is closely tied to atmospheric
temperature, falling and rising in phase with temperature at
the inception and termination of glacial episodes (Wuebbles
and Hayhoe, 2002). Brook et al. (2000) show that, following
each transition, temperature increased more rapidly than CH
4
concentration. Since biogenic CH
4
production and emission
from major sources (wetlands, land
fi
lls, rice agriculture and
biomass burning) are in
fl
uenced by climate variables such as
temperature and moisture, the effect of climate on emissions
from these sources is signi
fi
cant.
Several studies indicate a high sensitivity of wetland CH
4
emissions to temperature and water table. Before the 1990s,
elevated surface temperature and emissions from wetlands were
believed to contribute to the increase in global CH
4
emissions
(Walter and Heimann, 2001a,b; Christensen et al., 2003; Zhuang
et al., 2004). Observations indicate substantial increases in
CH
4
released from northern peatlands that are experiencing
permafrost melt (Christensen et al., 2004; Wickland et al.,
2006). Based on the relationship between emissions and
temperature at two wetland sites in Scotland, Chapman and
Thurlow (1996) predicted that CH
4
emissions would increase
by 17, 30 and 60% for warmings of 1.5°C, 2.5°C and 4.5°C
(warming above the site’s mean temperature during 1951 to
1980), respectively. A model simulation by Cao et al. (1998)
yielded a 19% emission increase under a uniform 2°C warming.
The combined effects of a 2°C warming and a 10% increase
in precipitation yielded an increase of 21% in emissions. In
most cases, the net emission depends on how an increase in
temperature affects net ecosystem production (NEP), as this is
the source of methanogenic substrates (Christensen et al., 2003),
and on the moisture regime of wetlands, which determines
if decomposition is aerobic or anaerobic. Emissions increase
under a scenario where an increase in temperature is associated
with increases in precipitation and NEP, but emissions decrease
if elevated temperature results in either reduced precipitation or
reduced NEP.
For a doubling in atmospheric CO
2
concentration, the GCM
of Shindell et al. (2004) simulates a 3.4°C warming. Changes
in the hydrological cycle due to this CO
2
doubling cause CH
4
emissions from wetlands to increase by 78%. Gedney et al.
(2004) also simulate an increase in CH
4
emissions from northern
wetlands due to an increase in wetland area and an increase in
CH
4
production due to higher temperatures. Zhuang et al. (2004)
use a terrestrial ecosystem model based on emission data for the
1990s to study how rates of CH
4
emission and consumption in
high-latitude soils of the NH (north of 45°N) have changed over
the past century (1900–2000) in response to observed change in
the region’s climate. They estimate that average net emissions
of CH
4
increased by 0.08 Tg yr
–1
over the 20th century. Their
decadal net CH
4
emission rate correlates with soil temperature
and water table depth.
In rice agriculture
,
climate factors that will likely in
fl
uence
CH
4
emission are those associated with plant growth. Plant
growth controls net emissions by determining how much substrate
will be available for either methanogenesis or methanotrophy
(Matthews and Wassmann, 2003). Sass et al. (2002) show that
CH
4
emissions correlate strongly with plant growth (height) in
a Texas rice
fi
eld. Any climate change scenario that results in an
increase in plant biomass in rice agriculture is likely to increase
CH
4
emissions (Xu et al., 2004). However, the magnitude of
increased emission depends largely on water management. For
example,
fi
eld drainage could signi
fi
cantly reduce emission due
to aeration of the soil (i.e., in
fl
ux of air into anaerobic zones that
subsequently suppresses methanogenesis, Li et al., 2002).
Past observations indicate large interannual variations in
CH
4
growth rates (Dlugokencky et al., 2001). The mechanisms
causing these variations are poorly understood and the role
of climate is not well known. Emissions from wetlands and
biomass burning may have contributed to emission peaks in
1993 to 1994 and 1997 to 1998 (Langenfelds et al., 2002; Butler
et al., 2004). Unusually warm and dry conditions in the NH
during ENSO periods increase biomass burning. Kasischke and
Bruhwiler (2002) attribute CH
4
releases of 3 to 5 Tg in 1998 to
boreal forest
fi
res in Eastern Siberia resulting from unusually
warm and dry conditions.
Meteorological conditions can affect global mean removal
rates (Warwick et al., 2002; Dentener et al., 2003a). Dentener
et al.
fi
nd that over the period 1979 to 1993, the primary effect
resulted from changes in OH distribution caused by variations in
tropical tropospheric water vapour. Johnson et al. (2001) studied
predictions of the CH
4
evolution over the 21st century and found
that there is also a substantial increase in CH
4
destruction due to
increases in the CH
4
+ OH rate coef
fi
cient in a warming climate.
There also appear to be signi
fi
cant interannual variations in the
active Cl sink, but a climate in
fl
uence has yet to be identi
fi
ed
(Allan et al., 2005). On the other hand, several model studies
indicate that CH
4
oxidation in soil is relatively insensitive to
temperature increase (Ridgwell at al., 1999; Zhuang et al.,
2004). A doubling of atmospheric CO
2
would likely change
the sink strength only marginally (in the range of –1 to
+3 Tg(CH
4
) yr
–1
; Ridgwell et al., 1999). However, any change
in climate that alters the amount and pattern of precipitation
may signi
fi
cantly affect the CH
4
oxidation capacity of soils. A
process-based model simulation indicated that CH
4
oxidation
strongly depends on soil gas diffusivity, which is a function of
soil bulk density and soil moisture content (Bogner et al., 2000;
Del Grosso et al., 2000).
Climate also affects the stability of CH
4
hydrates beneath
the ocean, where large amounts of CH
4
are stored (~4 ×10
6
Tg;
Buffett and Archer, 2004). The
δ
13
C values of ancient sea
fl
oor
carbonates reveal several hydrate dissociation events that appear
to have occurred in connection with rapid warming episodes in
the Earth’s history (Dickens et al., 1997; Dickens, 2001). Model
544
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
results indicate that these hydrate decomposition events occurred
too fast to be controlled by the propagation of the temperature
change into the sediments (Katz et al., 1999; Paull et al., 2003).
Additional studies infer other indirect and inherently more rapid
mechanisms such as enhanced migration of free gas, or reordering
of gas hydrates due to slump slides (Hesselbo et al., 2000; Jahren
et al., 2001; Kirschvink et al., 2003; Ryskin, 2003). Recent
modelling suggests that today’s sea
fl
oor CH
4
inventory would be
diminished by 85% with a warming of bottom water temperatures
by 3°C (Buffett and Archer, 2004). Based on this inventory, the
time-dependent feedback of hydrate destabilisation to global
warming has been addressed using different assumptions for
the time constant of destabilisation: an anthropogenic release of
2,000 GtC to the atmosphere could cause an additional release of
CH
4
from gas hydrates of a similar magnitude (
∼
2,000 Gt(CH
4
))
over a period of 1 to 100 kyr (Archer and Buffett, 2005). Thus,
gas hydrate decomposition represents an important positive CH
4
feedback to be considered in global warming scenarios on longer
time scales.
In summary, advances have been made since the TAR
in constraining estimates of CH
4
source strengths and in
understanding emission variations. These improvements
are attributed to increasing availability of worldwide
observations and improved modelling techniques. Emissions
from anthropogenic sources remain the major contributor to
atmospheric CH
4
budgets. Global emissions are likely not to
have increased since the time of the TAR, as nearly zero growth
rates in atmospheric CH
4
concentrations have been observed
with no signi
fi
cant change in the sink strengths.
7.4.2 Nitrogen
Compounds
The N cycle is integral to functioning of the Earth system and
to climate (Vitousek et al., 1997; Holland et al., 2005a). Over
the last century, human activities have dramatically increased
emissions and removal of reactive N to the global atmosphere
by as much as three to
fi
ve fold. Perturbations of the N cycle
affect the atmosphere climate system through production of
three key N-containing trace gases: N
2
O, ammonia (NH
3
) and
NO
x
(nitric oxide (NO) + nitrogen dioxide (NO
2
)). Nitrous
oxide is the fourth largest single contributor to positive
radiative forcing, and serves as the only long-lived atmospheric
tracer of human perturbations of the global N cycle (Holland et
al., 2005a). Nitrogen oxides have short atmospheric lifetimes
of hours to days (Prather et al., 2001). The dominant impact
of NO
x
emissions on the climate is through the formation of
tropospheric ozone, the third largest single contributor to
positive radiative forcing (Sections 2.3.6, 7.4.4). Emissions of
NO
x
generate indirect negative radiative forcing by shortening
the atmospheric lifetime of CH
4
(Prather 2002). Ammonia
contributes to the formation of sulphate and nitrate aerosols,
thereby contributing to aerosol cooling and the aerosol indirect
effect (Section 7.5), and to increased nutrient supply for the
carbon cycle (Section 7.5). Ammonium and NO
x
are removed
from the atmosphere by deposition, thus affecting the carbon
cycle through increased nutrient supply (Section 7.3.3.1.3).
Atmospheric concentrations of N
2
O have risen 16%, from
about 270 ppb during the pre-industrial era to 319 ppb in 2005
(Figure 7.16a). The average annual growth rate for 1999 to
2000 was 0.85 to 1.1 ppb yr
–1
, or about 0.3% per year (WMO,
2003). The main change in the global N
2
O budget since the
TAR is quanti
fi
cation of the substantial human-driven emission
of N
2
O (Table 7.7; Naqvi et al., 2000; Nevison et al., 2004;
Kroeze et al.,
2005; Hirsch et al., 2006). The annual source of
N
2
O from the Earth’s surface has increased by about 40 to 50%
over pre-industrial levels as a result of human activity (Hirsch
et al., 2006). Human activity has increased N supply to coastal
and open oceans, resulting in decreased O
2
availability and N
2
O
emissions (Naqvi et al., 2000; Nevison et al., 2004).
Since the TAR, both top-down and bottom-up estimates of
N
2
O have been re
fi
ned. Agriculture remains the single biggest
anthropogenic N
2
O source (Bouwman et al., 2002; Smith
and Conen, 2004; Del Grosso et al., 2005). Land use change
continues to affect N
2
O and NO emissions (Neill et al., 2005):
logging is estimated to increase N
2
O and NO emissions by 30
to 350% depending on conditions (Keller et al., 2005). Both
studies underscore the importance of N supply, temperature
and moisture as regulators of trace gas emissions. The
inclusion of several minor sources (human excreta, land
fi
lls
and atmospheric deposition) has increased the total bottom-up
budget to 20.6 TgN yr
–1
(Bouwman et al., 2002). Sources of
N
2
O now estimated since the TAR include coastal N
2
O
fl
uxes
of 0.2 TgN yr
–1
(±70%; Nevison et al., 2004) and river and
estuarine N
2
O
fl
uxes of 1.5 TgN yr
–1
(Kroeze et al., 2005).
Box model calculations show the additional river and estuarine
sources to be consistent with the observed rise in atmospheric
N
2
O (Kroeze et al., 2005).
Top-down estimates of surface sources use observed
concentrations to constrain total sources and their spatial
distributions. A simple calculation, using the present-day N
2
O
burden divided by its atmospheric lifetime, yields a global
stratospheric loss of about 12.5 ± 2.5 TgN yr
–1
. Combined with
the atmospheric increase, this loss yields a surface source of
16 TgN yr
–1
. An inverse modelling study of the surface
fl
ux
of N
2
O yields a global source of 17.2 to 17.4 TgN yr
–1
with
an estimated uncertainty of 1.4 (1 standard deviation; Hirsch
et al., 2006). The largest sources of N
2
O are from land at
tropical latitudes, the majority located north of the equator. The
Hirsch et al. inversion results further suggest that N
2
O source
estimates from agriculture and fertilizer may have increased
markedly over the last three decades when compared with an
earlier inverse model estimate (Prinn et al., 1990). Bottom-up
estimates, which sum individual source estimates, are more
evenly distributed with latitude and lack temporal variability.
However, there is clear consistency between top-down and
bottom-up global source estimates, which are 17.3 (15.8–18.4)
and 17.7 (8.5–27.7) TgN yr
–1
, respectively.
Concentrations of NO
x
and reduced nitrogen (NH
x
=
NH
3
+ ammonium ion (NH
4
+
)) are dif
fi
cult to measure because
the atmospheric lifetimes of hours to days instead of years
generate pronounced spatial and temporal variations in their
distributions. Atmospheric concentrations of NO
x
and NH
x
545
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Figure 7.16.
(a) Changes in the emissions of fuel combustion NO
x
and atmo-
spheric N
2
O mixing ratios since 1750. Mixing ratios of N
2
O provide the atmospheric
measurement constraint on global changes in the N cycle. (b) Changes in the indices
of the global agricultural N cycle since 1850: the production of manure, fertilizer
and estimates of crop N fi xation. For data sources see http://www-eosdis.ornl.gov/
(Holland et al., 2005b) and http://www.cmdl.noaa.gov/. Figure adapted from Holland
et al. (2005c).
vary more regionally and temporally than concentrations
of N
2
O. Total global NO
x
emissions have increased from an
estimated pre-industrial value of 12 TgN yr
–1
(Holland et al.,
1999; Galloway et al., 2004) to between 42 and 47 TgN yr
–1
in 2000 (Table 7.7). Lamarque et al. (2005a) forecast them to
be 105 to 131 TgN yr
–1
by 2100. The range of surface NO
x
emissions (excluding lightning and aircraft) used in the current
generation of global models is 33 to 45 TgN yr
–1
with small
ranges for individual sources. The agreement re
fl
ects the use
of similar inventories and parametrizations. Current estimates
of NO
x
emissions from fossil fuel combustion are smaller than
in the TAR.
Since the TAR, estimates of tropospheric NO
2
columns from
space by the Global Ozone Monitoring Experiment (GOME,
launched in 1995) and the SCanning Imaging Absorption
SpectroMeter for Atmospheric CHartographY (SCIAMACHY,
launched in 2002) (Richter and Burrows, 2002; Heue et al.,
2005) provide constraints on estimates of NO
x
emissions
(Leue et al., 2001). Martin et al. (2003a) use GOME data to
estimate a global surface source of NO
x
of 38 TgN yr
–1
for 1996
to 1997 with an uncertainty factor of 1.6. Jaeglé et al. (2005)
partition the surface NO
x
source inferred from GOME into 25.6
TgN yr
–1
from fuels, 5.9 TgN yr
–1
from biomass burning and
8.9 TgN yr
–1
from soils. Interactions between soil emissions
and scavenging by plant canopies have a signi
fi
cant impact
on soil NO
x
emissions to the free troposphere: the impact
may be greatest in subtropical and tropical regions where
emissions from fuel combustion are rising (Ganzeveld et al.,
2002). Boersma et al. (2005)
fi
nd that GOME data constrain
the global lightning NO
x
source for 1997 to the range 1.1 to 6.4
TgN yr
–1
. Comparison of the tropospheric NO
2
column of three
state-of-the-art retrievals from GOME for the year 2000 with
model results from 17 global atmospheric chemistry models
highlights signi
fi
cant differences among the various models
and among the three GOME retrievals (Figure 7.17, van Noije
et al., 2006). The discrepancies among the retrievals (10 to
50% in the annual mean over polluted regions) indicate that
the previously estimated retrieval uncertainties have a large
systematic component. Top-down estimates of NO
x
emissions
from satellite retrievals of tropospheric NO
2
are strongly
dependent on the choice of model and retrieval.
Knowledge of the spatial distribution of NO
x
emissions
has evolved signi
fi
cantly since the TAR. An Asian increase in
emissions has been compensated by a European decrease over
the past decade (Naja et al., 2003). Richter et al. (2005; see
also Irie et al., 2005) use trends for 1996 to 2004 observed by
GOME and SCIAMACHY to deduce a 50% increase in NO
x
emissions over industrial areas of China. Observations of
NO
2
in shipping lanes from GOME (Beirle et al., 2004) and
SCIAMACHY (Richter et al., 2004) give values at the low end
of emission inventories. Data from GOME and SCIAMACHY
further reveal large pulses of soil NO
x
emissions associated
with rain (Jaeglé et al., 2004) and fertilizer application (Bertram
et al., 2005).
All indices show an increase since pre-industrial times in the
intensity of agricultural nitrogen cycling, the primary source
of NH
3
emissions (Figure 7.16b and Table 7.7; Bouwman et
al., 2002). Total global NH
3
emissions have increased from an
estimated pre-industrial value of 11 TgN yr
–1
to 54 TgN yr
–1
for 2000 (Holland et al., 1999; Galloway et al., 2004), and are
projected to increase to 116 TgN yr
–1
by 2050.
The primary sink for NH
x
and NO
x
and their reaction
products is wet and dry deposition. Estimates of the removal
rates of both NH
x
and NO
x
are provided by measurements of
546
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Table 7.7.
Global sources (TgN yr
–1
) of NO
x
, NH
3
and N
2
O for the 1990s.
Source
NO
x
NH
3
N
2
O
TAR
a
AR4
b
TAR
a
AR4
a
TAR
c
AR4
Anthropogenic sources
Fossil fuel combustion
& industrial processes
33
(20–24)
25.6
(21–28)
0.3
(0.1–0.5)
2.5
d
1.3/0.7
(0.2–1.8)
0.7
(0.2–1.8)
d
Aircraft
0.7
(0.2–0.9)
–
e
(0.5–0.8)
-
-
-
-
Agriculture
2.3
f
(0–4)
1.6
g
34.2
(16–48)
35
g
(16–48)
6.3/2.9
(0.9–17.9)
2.8
(1.7–4.8)
g
Biomass and biofuel
burning
7.1
(2–12)
5.9
(6–12)
5.7
(3–8)
5.4
d
(3–8)
0.5
(0.2–1.0)
0.7
(0.2–1.0)
g
Human excreta
–
–
2.6
(1.3–3.9)
2.6
g
(1.3–3.9)
–
0.2
g
(0.1–0.3)
h
Rivers, estuaries, coastal
zones
–
–
–
–
–
1.7
(0.5–2.9)
i
Atmospheric deposition
–
0.3
g
–
–
–
0.6
j
(0.3–0.9)
h
Anthropogenic total
43.1
33.4
42.8
45.5
8.1/4.1
6.7
Natural sources
Soils under natural
vegetation
3.3
f
(3–8)
7.3
j
(5–8)
2.4
(1–10)
2.4
g
(1–10)
6.0/6.6
(3.3–9.9)
6.6
(3.3–9.0)
g
Oceans
–
–
8.2
(3–16)
8.2
g
(3–6)
3.0/3.6
(1.0–5.7)
3.8
(1.8–5.8)
k
Lightning
5
(2–12)
1.1–6.4
(3–7)
–
–
–
–
Atmospheric chemistry
<0.5
–
–
–
0.6
(0.3–1.2)
0.6
(0.3–1.2)
c
Natural total
8.8
8.4–13.7
10.6
10.6
9.6/10.8
11.0
Total sources
51.9
(27.2–60.9)
41.8–47.1
(37.4–57.7)
53.4
(40–70)
56.1
(26.8–78.4)
17.7/14.9
(5.9–37.5)
17.7
(8.5–27.7)
Notes:
a
Values from the TAR: NO
x
from Table 4.8 with ranges from Tables 4.8 and 5.2; NH
3
from Table 5.2, unless noted.
b
Parentheses show the range of emissions used in the model runs described in Table 7.9. See text for explanation. Where possible, the best estimate NO
x
emission
is based on satellite observations. None of the model studies includes the NO
x
source from oxidation of NH
3
, which could contribute up to 3 TgN yr
–1
. The source of
NO
x
from stratosphere-troposphere exchange is less than 1 TgN yr
–1
in all models, which is well constrained from observations of N
2
O-NO
x
correlations in the lower
stratosphere (Olsen et al., 2001).
c
Values are from the TAR, Table 4.4; Mosier et al. (1998); Kroeze et al. (1999)/Olivier et al. (1998): a single value indicates agreement between the sources and
methodologies of the different studies.
d
Van Aardenne et al. (2001), range from the TAR.
e
The aircraft source is included in the total for industrial processes. The parentheses indicate values used in model runs.
f
The total soil NO
x
emissions estimate of 5.6 provided in Table 4.8 of the TAR was distributed between agriculture and soil NO
x
according to the proportions provided
in the TAR, Table 5.2.
g
Bouwman et al. (2001, Table 1); Bouwman et al. (2002) for the 1990s; range from the TAR or calculated as ±50%.
h
Estimated as ±50%.
i
Kroeze et al. (2005); Nevison et al. (2004); estimated uncertainty is ±70% from Nevison et al. (2004).
j
All soils, minus the fertilized agricultural soils indicated above.
k
Nevison et al. (2003, 2004), combining the uncertainties in ocean production and oceanic exchange.
wet deposition over the USA and Western Europe to quantify
acid rain inputs (Hauglustaine et al., 2004; Holland et al.,
2005a; Lamarque et al., 2005a). Chemical transport models
represent the wet and dry deposition of NO
x
and NH
x
and their
reaction products. A study of 29 simulations with 6 different
tropospheric chemistry models, focusing on present-day and
2100 conditions for NO
x
and its reaction products, projects an
average increase in N deposition over land by a factor of 2.5 by
2100 (Lamarque et al., 2005b), mostly due to increases in NO
x
emissions. Nitrogen deposition rates over Asia are projected to
increase by a factor of 1.4 to 2 by 2030. Climate contributions
to the changes in oxidized N deposition are limited by the
models’ ability to represent changes in precipitation patterns.
An intercomparison of 26 global atmospheric chemistry models
demonstrates that current scenarios and projections are not
suf
fi
cient to stabilise or reduce N deposition or ozone pollution
before 2030 (Dentener et al., 2006).
547
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.4.3. Molecular
Hydrogen
Increased interest in atmospheric H
2
is due to its potential
role as an indirect greenhouse gas (Derwent et al., 2001) and
expected perturbations of its budget in a prospective ‘hydrogen
economy’ (Schultz et al., 2003; Tromp et al., 2003; Warwick et
al., 2004). Potential consequences of increased H
2
emissions
include a reduction of global oxidizing capacity (presently H
2
constitutes 5 to 10% of the global average OH sink, Schultz
et al., 2003) and increased formation of water vapour, which
could lead to increased cirrus formation in the troposphere
and increased polar stratospheric clouds (PSCs) and additional
cooling in the stratosphere, thereby leading to more ef
fi
cient
ozone depletion (Tromp et al., 2003).
Studies of the global tropospheric H
2
budget (see Table
7.8) generally agree on a total source strength of between 70
and 90 Tg(H
2
)
yr
–1
, which is approximately balanced by its
sinks. About half of the H
2
is produced in the atmosphere via
photolysis of formaldehyde (CH
2
O), which itself originates
from the oxidation of CH
4
and other volatile organic
compounds. The other half stems mostly from the combustion
of fossil fuels (e.g., car exhaust) and biomass burning. About
10% of the global H
2
source is due to ocean biochemistry
and N
fi
xation in soils. Presently, about 50 Tg(H
2
) yr
–1
are
produced in the industrial sector, mostly for the petrochemical
industry (e.g., re
fi
neries) (Lovins, 2003). Evaporative losses
of industrial H
2
are generally assumed to be negligible (Zittel
and Altmann, 1996). The dominant sink of atmospheric H
2
is
deposition with catalytic destruction by soil microorganisms
and possibly enzymes (Conrad and Seiler, 1981). The seasonal
cycle of observed H
2
concentrations implies an atmospheric
lifetime of about 2 years (Novelli et al., 1999; Simmonds et
al., 2000; Hauglustaine and Ehhalt, 2002), whereas the lifetime
with respect to OH oxidation is 9 to 10 years, which implies
that the deposition sink is about three to four times as large as
the oxidation. Loss of H
2
to the stratosphere and its subsequent
escape to space is negligible for the tropospheric H
2
budget,
because the budgets of the troposphere and stratosphere are
largely decoupled (Warneck, 1988).
Estimates of H
2
required to fuel a future carbon-free energy
system are highly uncertain and depend on the technology as
well as the fraction of energy that might be provided by H
2
. In
the future, H
2
emissions could at most double: the impact on
global oxidizing capacity and stratospheric temperatures and
ozone concentrations is estimated to be small (Schultz et al.,
2003; Warwick et al., 2004). According to Schultz et al. (2003),
the side effects of a global H
2
economy could have a stronger
impact on global climate and air pollution. Global oxidizing
capacity is predominantly controlled by the concentration of
NO
x
. Large-scale introduction of H
2
-powered vehicles would
lead to a signi
fi
cant decrease in global NO
x
emissions, leading
to a reduction in OH of the order of 5 to 10%. Reduced NO
x
levels could also signi
fi
cantly reduce tropospheric ozone
concentrations in urban areas. Despite the expected large-
scale use of natural gas for H
2
production, the impact of a H
2
economy on the global CH
4
budget is likely to be small, except
for the feedback between reduced oxidizing capacity (via NO
x
reduction) and CH
4
lifetime.
7.4.4 Global
Tropospheric
Ozone
7.4.4.1
Present-Day Budgets of Ozone and its Precursors
Tropospheric ozone is (after CO
2
and CH
4
) the third most
important contributor to greenhouse radiative forcing. Trends
over the 20th century are discussed in Chapter 2. Ozone is
produced in the troposphere by photochemical oxidation of
CO, CH
4
and non-methane VOCs (NMVOCs) in the presence
Figure 7.17.
Tropospheric column NO
2
from (a) satellite measurements and (b) atmospheric chemistry models. The maps represent ensemble average annual mean tropospher-
ic NO
2
column density maps for the year 2000. The satellite retrieval ensemble comprises three state-of-the-art retrievals from GOME; the model ensemble includes 17 global
atmospheric chemistry models. These maps were obtained after smoothing the data to a common horizontal resolution of 5° × 5° (adapted from van Noije et al., 2006).
548
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
of NO
x
. Stratosphere-troposphere exchange (STE) is another
source of ozone to the troposphere. Loss of tropospheric ozone
takes place through chemical reactions and dry deposition.
Understanding of tropospheric ozone and its relationship to
sources requires three-dimensional tropospheric chemistry
models that describe the complex nonlinear chemistry involved
and its coupling to transport.
The past decade has seen considerable development in
global models of tropospheric ozone, and the current generation
of models can reproduce most climatological features of ozone
observations. The TAR reported global tropospheric ozone
budgets from 11 models in the 1996 to 2000 literature. Table 7.9
presents an update to the post-2000 literature, including a recent
intercomparison of 25 models (Stevenson et al., 2006). Models
concur that chemical production and loss are the principal terms
in the global budget. Although STE is only a minor term in
the global budget, it delivers ozone to the upper troposphere
where its lifetime is particularly long (about one month, limited
by transport to the lower troposphere) and where it is of most
importance from a radiative forcing perspective.
The post-2000 model budgets in Table 7.9 show major
differences relative to the older generation TAR models:
on average a 34% weaker STE, a 35% stronger chemical
production, a 10% larger tropospheric ozone burden, a 16%
higher deposition velocity and a 10% shorter chemical lifetime.
It is now well established that many of the older studies
overestimated STE, as observational constraints in the lower
stratosphere impose an STE ozone
fl
ux of 540 ± 140 Tg yr
–1
(Gettelman et al., 1997; Olsen et al., 2001). Overestimation of the
STE
fl
ux appears to be most serious in models using assimilated
meteorological data, due to the effect of assimilation on vertical
motions (Douglass et al., 2003; Schoeberl et al., 2003; Tan et
al., 2004; Van Noije et al., 2004). The newer models correct for
this effect by using dynamic
fl
ux boundary conditions in the
tropopause region (McLinden et al., 2000) or by relaxing model
results to observed climatology (Horowitz et al., 2003). Such
corrections, although matching the global STE
fl
ux constraints,
may still induce errors in the location of the transport (Hudman
et al., 2004) with implications for the degree of stratospheric
in
fl
uence on tropospheric concentrations (Fusco and Logan,
2003).
The faster chemical production and loss of ozone in the
current generation of models could re
fl
ect improved treatment
of NMVOC sources and chemistry (Houweling et al., 1998),
ultraviolet (UV) actinic
fl
uxes (Bey et al., 2001) and deep
convection (Horowitz et al., 2003), as well as higher NO
x
emissions (Stevenson et al., 2006). Subtracting ozone chemical
production and loss terms in Table 7.9 indicates that the
current generation of models has net production of ozone in
the troposphere, while the TAR models had net loss, re
fl
ecting
the decrease in STE. Net production is not a useful quantity
in analysing the ozone budget because (1) it represents only a
small residual between production and loss and (2) it re
fl
ects
a balance between STE and dry deposition, both of which are
usually parametrized in models.
Detailed budgets of ozone precursors were presented in
the TAR. The most important precursors are CH
4
and NO
x
(Wang et al., 1998; Grenfell et al., 2003; Dentener et al., 2005).
Methane is in general not simulated explicitly in ozone models
and is instead constrained from observations. Nitrogen oxides
are explicitly simulated and proper representation of sources
and chemistry is critical for the ozone simulation. The lightning
source is particularly uncertain (Nesbitt et al., 2000; Tie et al.,
2002), yet is of great importance because of the high production
ef
fi
ciency of ozone in the tropical upper troposphere. The range
of the global lightning NO
x
source presently used in models
(3–7 TgN yr
–1
) is adjusted to match atmospheric observations
of ozone and NO
x
, although large model uncertainties in deep
Table 7.8.
Summary of global budget studies of atmospheric H
2
(Tg(H
2
) yr
–1
).
Sanderson et
al. (2003a)
Hauglustaine
and Ehhalt
(2002)
Novelli et al.
(1999)
Ehhalt (1999)
Warneck (1988)
Seiler and
Conrad (1987)
Sources
Oxidation of CH
4
and VOC
30.2
31
40 ± 16
35 ± 15
50
40 ± 15
Fossil fuel combustion
20
16
15 ± 10
15 ± 10
17
20 ± 10
Biomass burning
20
13
16 ± 11
16 ± 5
15
20 ± 10
N
2
fi xation
4
5
3 ± 1
3 ± 2
3
3 ± 2
Ocean release
4
5
3 ± 2
3 ± 2
4
4 ± 2
Volcanoes
–
–
–
–
0.2
–
Total
78.2
70
77 ± 16
71 ± 20
89
87
Sinks
Deposition
58.3
55
56 ± 41
40 ± 30
78
90 ± 20
Oxidation by OH
17.1
15
19 ± 5
25 ± 5
11
8 ± 3
Total
74.4
70
75 ± 41
65 ± 30
89
98
549
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Table 7.9.
Global budgets of tropospheric ozone (Tg yr
–1
) for the present-day atmosphere
a
.
Reference
Model
b
Stratosphere-
Troposphere
Exchange
Chemical
Production
c
Chemical
Loss
c
Dry
Deposition
Burden
(Tg)
Lifetime
d
(days)
TAR
e
11 models
770 ± 400
3420 ± 770
3470 ± 520
770 ± 180
300 ± 30
24 ± 2
Lelieveld and
Dentener (2000)
TM3
570
3310
3170
710
350
33
Bey et al. (2001)
GEOS-Chem
470
4900
4300
1070
320
22
Sudo et al. (2002b)
CHASER
593
4895
4498
990
322
25
Horowitz et al. (2003)
MOZART-2
340
5260
4750
860
360
23
Von Kuhlmann et al.
(2003)
MATCH-MPIC
540
4560
4290
820
290
21
Shindell et al. (2003)
GISS
417
NR
f
NR
1470
349
NR
Hauglustaine et al.
(2004)
LMDz-INCA
523
4486
3918
1090
296
28
Park et al. (2004)
UMD-CTM
480
NR
NR
1290
340
NR
Rotman et al. (2004)
IMPACT
660
NR
NR
830
NR
NR
Wong et al. (2004)
SUNY/UiO GCCM
600
NR
NR
1100
376
NR
Stevenson et al.
(2004)
STOCHEM
395
4980
4420
950
273
19
Wild et al. (2004)
FRSGC/UCI
520
4090
3850
760
283
22
Folberth et al. (2006)
LMDz-INCA
715
4436
3890
1261
303
28
Stevenson et al.
(2006)
25 models
520 ± 200
5060 ± 570
4560 ± 720
1010 ± 220
340 ± 40
22 ± 2
Notes:
a
From global model simulations describing the atmosphere of the last decade of the 20th century.
b
TM3: Royal Netherlands Meteorological Institute (KNMI) chemistry transport model; GEOS-Chem: atmospheric composition model driven by observations from the
Goddard Earth Observing System; CHASER: Chemical AGCM for Study of Atmospheric Environment and Radiative Forcing; MOZART-2: Model for (tropospheric)
Ozone and Related Tracers; MATCH-MPIC: Model of Atmospheric Transport and Chemistry – Max Planck Institute for Chemistry; GISS: Goddard Institute for Space
Studies chemical transport model; LMDz-INCA: Laboratoire de Météorologie Dynamique GCM-Interactive Chemistry and Aerosols model; UMD-CTM: University
of Maryland Chemical Transport Model; IMPACT: Integrated Massively Parallel Atmospheric Chemistry Transport model; SUNY/UiO GCCM: State University of
New York/University of Oslo Global Tropospheric Climate-Chemistry Model; STOCHEM: Hadley Centre global atmospheric chemistry model; FRSGC/UCI: Frontier
Research System for Global Change/University of California at Irvine chemical transport model.
c
Chemical production and loss rates are calculated for the odd oxygen family, usually defi ned as O
x
= ozone + O + NO
2
+ 2NO
3
+ 3 dinitrogen pentoxide (N
2
O
5
)
+ pernitric acid (HNO
4
) + peroxyacylnitrates (and sometimes nitric acid; HNO
3
), to avoid accounting for rapid cycling of ozone with short-lived species that have
little implication for its budget. Chemical production is mainly contributed by reactions of NO with peroxy radicals, while chemical loss is mainly contributed by the
oxygen radical in the 1D excited state (O(
1
D)) plus water (H
2
O) reaction and by the reactions of ozone with the hydroperoxyl radical (HO
2
), OH, and alkenes.
d
Calculated as the ratio of the burden to the sum of chemical and deposition losses.
e
Means and standard deviations for 11 global model budgets from the 1996 to 2000 literature reported in the TAR. The mean budget does not balance exactly
because only nine chemical transport models reported their chemical production and loss statistics.
f
Not reported.
convection and lightning vertical distributions detract from the
strength of this constraint. Process-based models tend to predict
higher lightning emissions (5–20 TgN yr
–1
; Price et al., 1997).
Other signi
fi
cant precursors for tropospheric ozone
are CO and NMVOCs, the most important of which is
biogenic isoprene. Satellite measurements of CO from the
Measurements of Pollution in the Troposphere (MOPITT)
instrument launched in 1999 (Edwards et al., 2004) have
provided important new constraints for CO emissions, pointing
in particular to an underestimate of Asian sources in current
inventories (Kasibhatla et al., 2002; Arellano et al., 2004; Heald
et al., 2004; Petron et al., 2004), as con
fi
rmed also by aircraft
observations of Asian out
fl
ow (Palmer et al., 2003a; Allen et al.,
2004). Satellite measurements of formaldehyde columns from
the GOME instrument (Chance et al., 2000) have been used
to place independent constraints on isoprene emissions and
indicate values generally consistent with current inventories,
although with signi
fi
cant regional discrepancies (Palmer et al.,
2003b; Shim et al., 2005).
A few recent studies have examined the effect of aerosols
on global tropospheric ozone involving both heterogeneous
chemistry and perturbations to actinic
fl
uxes. Jacob (2000)
reviewed the heterogeneous chemistry involved. Hydrolysis of
dinitrogen pentoxide (N
2
O
5
) in aerosols is a well-known sink
for NO
x
, but other processes involving reactive uptake of the
hydroperoxyl radical (HO
2
), NO
2
and ozone itself could also
be signi
fi
cant. Martin et al. (2003b)
fi
nd that including these
processes along with effects of aerosols on UV radiation in
550
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
a global Chemical Transport Model (CTM) reduced ozone
production rates by 6% globally, with larger effects over aerosol
source regions.
Although the current generation of tropospheric ozone
models is generally successful in describing the principal
features of the present-day global ozone distribution, there is
much less con
fi
dence in the ability to reproduce the changes
in ozone associated with perturbations of emissions or climate.
There are major discrepancies with observed long-term trends
in ozone concentrations over the 20th century (Hauglustaine
and Brasseur, 2001; Mickley et al., 2001; Shindell and Favulegi,
2002; Shindell et al., 2003; Lamarque et al., 2005c), including
after 1970 when the reliability of observed ozone trends is high
(Fusco and Logan, 2003). Resolving these discrepancies is
needed to establish con
fi
dence in the models.
7.4.4.2
Effects of Climate Change
Climate change can affect tropospheric ozone by modifying
emissions of precursors, chemistry, transport and removal
(European Commission, 2003). These and other effects are
discussed below. They could represent positive or negative
feedbacks to climate change.
7.4.4.2.1
Effects on emissions
Climate change affects the sources of ozone precursors
through physical response (lightning), biological response
(soils, vegetation, biomass burning) and human response
(energy generation, land use, agriculture). It is generally
expected that lightning will increase in a warmer climate (Price
and Rind, 1994a; Brasseur et al., 2005; Hauglustaine et al.,
2005), although a GCM study by Stevenson et al. (2006) for the
2030 climate
fi
nds no global increase but instead a shift from
the tropics to mid-latitudes. Perturbations to lightning could
have a large effect on ozone in the upper troposphere (Toumi
et al., 1996; Thompson et al., 2000; Martin et al., 2002; Wong
et al., 2004). Mickley et al. (2001)
fi
nd that observed long-term
trends in ozone over the past century might be explainable by
an increase in lightning.
Biomass burning in the tropics and at high latitudes is likely
to increase with climate change, both as a result of increased
lightning and as a result of increasing temperatures and dryness
(Price and Rind, 1994b; Stocks et al., 1998; A. Williams et
al., 2001; Brown et al., 2004). Biomass burning is known to
make a large contribution to the budget of ozone in the tropical
troposphere (Thompson et al., 1996), and there is evidence
that boreal forest
fi
res can enhance ozone throughout the
extratropical NH (Jaffe et al., 2004). With climate warming, it is
likely that boreal
fi
res will increase due to a shorter duration of
the seasonal snowpack and decreased soil moisture (Kasischke
et al., 1995).
Biogenic VOC emissions may be highly sensitive to climate
change. The most important global ozone precursors are CH
4
and isoprene. The effect of climate change on CH
4
is discussed
in Section 7.4.1. The effect on NMVOCs was examined by
Constable et al. (1999), Sanderson et al. (2003b), and Lathière
et al. (2005). Although biogenic NMVOC emissions increase
with increasing temperature, all three studies concur that
climate-driven changes in vegetation types unfavourable to
isoprene emissions (notably the recession of tropical forests)
would partly compensate for the effect of warming in terms of
ozone generation.
7.4.4.2.2
Effects on chemistry
Changes in temperature, humidity and UV radiation
intensity brought about by climate change could affect ozone
signi
fi
cantly. Simulations with GCMs by Stevenson et al.
(2000) and Grewe et al. (2001) for the 21st century indicate
a decrease in the lifetime of tropospheric ozone as increasing
water vapour enhances the dominant ozone sink from the
oxygen radical in the 1D excited state (O(
1
D)) plus water
(H
2
O) reaction. Stevenson et al. (2006)
fi
nd similar results in an
intercomparison of nine models for 2030 compared with 2000
climate. However, regional ozone pollution may increase in the
future climate as a result of higher temperatures (see Section
7.6, Box 7.4).
7.4.4.2.3
Effects on transport
Changes in atmospheric circulation could have a major effect
on tropospheric ozone. Studies using GCMs concur that STE
should increase in the future climate because of the stronger
Brewer-Dobson stratospheric circulation (Sudo et al., 2002a;
Collins et al., 2003; Zeng and Pyle, 2003; Hauglustaine et al.,
2005; Stevenson et al., 2005). Changes in vertical transport
within the troposphere are also important, in view of the
rapid increase in both ozone production ef
fi
ciency and ozone
lifetime with altitude. Convection is expected to intensify as
climate warms (Rind et al., 2001), although this might not be
the case in the tropics (Stevenson et al., 2005). The implications
are complex, as recently discussed by Pickering et al. (2001),
Lawrence et al. (2003), Olivié et al. (2004), Doherty et al.
(2005) and Li et al. (2005). On the one hand, convection brings
down ozone-rich air from the upper troposphere to the lower
troposphere where it is rapidly destroyed, and replaces it with
low-ozone air. On the other hand, injection of NO
x
to the upper
troposphere greatly increases its ozone production ef
fi
ciency.
7.4.5 The
Hydroxyl
Radical
The hydroxyl radical (OH) is the primary cleansing agent
of the lower atmosphere, providing the dominant sink for
many greenhouse gases (e.g., CH
4
, hydrochloro
fl
uorocarbons
(HCFCs), hydro
fl
uorocarbons) and pollutants (e.g., CO, non-
methane hydrocarbons). Steady-state lifetimes of these trace
gases are determined by the morphology of their atmospheric
distribution, the kinetics of their reaction with OH and
the OH distribution. Local abundance of OH is controlled
mainly by local abundances of NO
x
, CO, CH
4
and higher
hydrocarbons, ozone, water vapour, as well as the intensity of
solar UV radiation at wavelengths shorter than 0.310
μ
m. New
laboratory and
fi
eld work also shows signi
fi
cant formation of
O(
1
D) from ozone photolysis in the wavelength range between
551
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
0.310
μ
m and 0.350
μ
m (Matsumi et al., 2002; Hofzumahaus
et al., 2004). The primary source of tropospheric OH is a pair
of reactions starting with the photodissociation of ozone by
solar UV radiation.
Additionally, in the remote, and in particular upper,
troposphere, photodissociation of oxygenated volatile organic
chemicals such as peroxides, acetone and other ketones, alcohols,
and aldehydes may be the dominant sources of OH radical (e.g.,
Müller and Brasseur, 1999; Collins et al., 1999; Jaeglé et al.,
2001; Tie et al., 2003; Singh et al., 2004). Over continents,
measurements in the lower troposphere suggest that processing
of unsaturated hydrocarbons or photolysis of carbonyls can
also sustain a large pool of radicals (e.g., Handisides et al.,
2003; Heard et al., 2004). Furthermore, the net formation of
OH by photolysis of nitrous acid (HONO) was found to be the
dominant OH radical source in urban atmospheres (e.g., Ren
et al., 2003) and in a forest canopy (Kleffmann et al., 2005).
The hydroxyl radical reacts with many atmospheric trace
gases, in most cases as the
fi
rst and rate-determining step of a
reaction chain that leads to more or less complete oxidation of
the compound. These chains often lead to formation of HO
2
,
which then reacts with ozone or NO to recycle back to OH.
Tropospheric OH and HO
2
are lost through radical-radical
reactions leading to the formation of peroxides or with NO
2
to
form nitric acid (HNO
3
). Sources and sinks of OH involve most
of the fast photochemistry of the troposphere.
7.4.5.1
Changes in the Hydroxyl Radical Over Time
7.4.5.1.1
Impact of emissions
Because of its dependence on CH
4
and other pollutants,
tropospheric OH is also expected to have changed since the
pre-industrial era and to change in the future. Pre-industrial OH
is likely to have been different than today, but because of the
counteracting effects of higher CO and CH
4
(decreasing OH)
and increased NO
x
and ozone (increasing OH) there is still
little consensus on the magnitude of this change. Several model
studies suggest a decline in weighted global mean OH from
pre-industrial time to the present of less than 10% (Shindell
et al., 2001; Lelieveld et al., 2002a; Lamarque et al., 2005a).
Other studies have reported larger decreases in global OH
of 16% (Mickley et al., 1999), 25% (Wong et al., 2004) and
33% (Hauglustaine and Brasseur, 2001). The model study by
Lelieveld et al. (2002b) suggests that during the past century,
OH concentration decreased substantially in the marine
troposphere through reaction with CH
4
and CO. However, on
a global scale it has been compensated by an increase over the
continents associated with strong emissions of NO
x
.
Karlsdottir and Isaksen (2000) used a three-dimensional
CTM accounting for varying NO
x
, CO and NMVOC emissions
and found a positive trend in OH of 0.43% yr
–1
over the period
1980 to 1996. Dentener et al.
(2003a,b), with a three-dimensional
CTM accounting for varying emissions of ozone precursors
and CH
4
, meteorology and column ozone, derive a positive
trend of 0.26% yr
–1
over the 1979 to 1993 period. J. Wang et
al. (2004) also use a three-dimensional CTM accounting for
interannual variations in CH
4
and CO emissions, transport and
column ozone to analyse the trend in CH
4
from 1988 to 1997.
They do not account for interannual variability of a number of
other variables that affect OH such as concentrations of NO
x
,
tropospheric ozone and NMVOCs. They also derive a positive
trend in OH over the period considered of 0.63% yr
–1
. Their
calculated trend in OH is associated primarily with the negative
trend in the overhead column ozone over the period considered
and the trend is reduced to 0.16% yr
–1
when the total ozone
column is held constant.
Future changes in OH depend on relative changes in
hydrocarbons compared with NO
x
abundances. In the TAR,
Prather et al.
(2001), using scenarios reported in the IPCC
SRES (IPCC, 2000) and on the basis of a comparison of results
from 14 models, predicted that global OH could decrease by
10 to 18% by 2100 for
fi
ve emission scenarios and increase by
5% for one scenario (which assumes large decreases in CH
4
and other ozone precursor emissions). Based on a different
emission scenario for future emissions, Wang and Prinn (1999)
also predicted an OH decrease of 16 ± 3% in 2100.
7.4.5.1.2
Effects of climate change
In addition to the emission changes, future increases in
greenhouse gases could also induce changes in OH, arising
through direct participation in OH-controlling chemistry and
indirectly through stratospheric ozone changes that could increase
solar UV radiation in the troposphere. OH will also be affected
by changes in temperature, humidity and clouds or climate
change effects on biogenic emissions of CH
4
and other ozone
precursors. Changes in tropospheric water could have important
chemical repercussions. The reaction between water vapour and
electronically excited oxygen atoms constitutes the major source
of tropospheric OH. So, in a warmer climate characterised by
increased speci
fi
c humidity, the abundance of OH is expected to
increase. This effect was proposed by Pinto and Khalil (1991)
to explain the variation of OH during the cold dry Last Glacial
Maximum (LGM). It was quanti
fi
ed by Martinerie et al. (1995)
who calculated that the global mean OH concentration during
the LGM was 7% lower than at present because the atmospheric
water vapour concentration was lower during that period. Valdes
et al. (2005) estimate that the cold and dry LGM climate was
responsible for a 7% decrease in global OH. Brasseur et al
.
(1998)
and Johnson et al. (1999) estimated that in a warmer (doubled
atmospheric CO
2
) climate, the global and annual mean OH
concentration would increase by 7% and 12.5%, respectively.
More recently, Hauglustaine et al. (2005) use a climate-chemistry
three-dimensional model to estimate a 16% reduction in global
OH from the present day to 2100 accounting solely for changes
in surface emissions. The effect of climate change and mainly of
increased water vapour in this model is to increase global OH by
13%. In this study, the competing effects of emissions and climate
change maintain the future global average OH concentration
close to its present-day value. The importance of the water vapour
distribution to global OH is illustrated by Lamarque et al. (2005a),
who show that under reduced aerosol emissions, a warmer and
moister climate signi
fi
cantly increases global OH concentration.
552
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Changes in lightning NO
x
emissions in a warmer climate
may also affect OH. Labrador et al. (2004) show that global OH
is sensitive to the magnitude of lightning NO
x
emissions, and
increases by 10% and 23% when global lightning is increased
by a factor of 2 and 4, respectively, from a 5 TgN yr
–1
best
estimate. Similar sensitivity of global OH to the lightning
source was estimated by Wang et al. (1998), who calculated a
10.6% increase in OH for a doubling of the source (from 3 to 6
TgN yr
–1
). Regarding the large uncertainty about lightning
emissions and the sensitivity of OH to the total amount of N
emitted, an improved understanding of this source appears
important for the ability to simulate OH accurately over time.
7.4.5.2
Consequences for Lifetimes
7.4.5.2.1 Lifetime
de
fi
nition
The global instantaneous atmospheric lifetime of a trace gas
in the atmosphere is obtained by integrating the loss frequency
l
over the atmospheric domain considered. The integral must
be weighted by the distribution of the trace gas on which the
sink processes act. Considering a distribution of the trace gas
C
(
x
,
y
,
z
,
t
), a global instantaneous lifetime derived from the
budget can be de
fi
ned as:
Ï„
global
=
∫
C
d
v /
∫
C
l
d
v
(7.4)
where
d
v
is an atmospheric volume element. This expression
can be averaged over one year to determine the global and
annual mean lifetime. The global atmospheric lifetime (also
called ‘burden lifetime’ or ‘turnover lifetime’) characterises the
time required to turn over the global atmospheric burden.
The global atmospheric lifetime characterises the time
to achieve an
e
-fold decrease of the global atmospheric
burden. Unfortunately
Ï„
global
is a constant only in very limited
circumstances. In the case where the loss rate depends on
the burden, the perturbation or pulse decay lifetime (
Ï„
pert
) is
introduced (see Velders et al., 2005). The perturbation lifetime
is used to determine how a one-time pulse emission may decay
as a function of time as needed for the calculation of Global
Warming Potentials (GWPs). The perturbation lifetime can be
distinctly different from the global atmospheric lifetime. For
example, if the CH
4
abundance increases above its present-day
value due to a one-time emission, the time it takes for CH
4
to
decay back to its background value is longer than its global
unperturbed atmospheric lifetime. This delay occurs because the
added CH
4
will cause a suppression of OH, in turn increasing
the background CH
4
. Such feedbacks cause the decay time of a
perturbation (
Ï„
pert
) to differ from the global atmospheric lifetime
(
Ï„
global
). In the limit of small perturbations, the relation between
the perturbation lifetime of a gas and its global atmospheric
lifetime can be derived from a simple budget relationship as
Ï„
pert
=
Ï„
global
/ (1–
f
), where the sensitivity coef
fi
cient
f
=
d
ln(
Ï„
global
) /
d
ln(
B
). Prather et al.
(2001) estimated the
feedback of CH
4
to tropospheric OH and its lifetime and
determined a sensitivity coef
fi
cient
f
= 0.28, giving a ratio
Ï„
pert
/
Ï„
global
of 1.4. Stevenson et al. (2006), from 25 CTMs,
calculate an ensemble mean and 1 standard deviation
uncertainty in present-day CH
4
global lifetime
Ï„
global
of 8.7 ±
1.3 years, which is the AR4 updated value. The corresponding
perturbation lifetime that should be used in the GWP calculation
is 12 ± 1.8 years.
Perturbation lifetimes can be estimated from global models by
simulating the injection of a pulse of gas and tracking the decay of
the added amount. The pulse of added CO, HCFCs or hydrocarbons,
by causing the concentration of OH to decrease and thus the lifetime
of CH
4
to increase temporarily, causes a buildup of CH
4
while the
added burden of the gas persists. Thus, changes in the emissions of
short-lived gases can generate long-lived perturbations as shown
in global models (Derwent et al., 2001; Wild et al., 2001; Collins
et al., 2002). Changes in tropospheric ozone accompany the CH
4
decay on a 12-year time scale as an inherent component of this
mode, a key example of chemical coupling in the troposphere.
Any chemically reactive gas, whether a greenhouse gas or not,
will produce some level of indirect greenhouse effect through its
impact on atmospheric chemistry.
7.4.5.2.2 Changes in lifetime
Since OH is the primary oxidant in the atmosphere of many
greenhouse gases including CH
4
and hydrogenated halogen
species, changes in OH will directly affect their lifetime in the
atmosphere and hence their impact on the climate system. Recent
studies show that interannual variations in the chemical removal
of CH
4
by OH have an important impact on the variability of
the CH
4
growth rate (Johnson et al., 2002; Warwick et al.,
2002; J. Wang et al., 2004). Variations in CH
4
oxidation by OH
contribute to a signi
fi
cant fraction of the observed variations
in the annual accumulation rate of CH
4
in the atmosphere. In
particular, the 1992 to 1993 anomaly in the CH
4
growth rate
can be explained by
fl
uctuations in OH and wetland emissions
after the eruption of Mt. Pinatubo (J. Wang et al., 2004). CH
4
variability simulated by Johnson et al. (2002), resulting only
from OH sink processes, also indicates that the ENSO cycle
is the largest component of that variability. These
fi
ndings are
consistent with the variability of global OH reconstructed by
Prinn et al. (2005), Manning and Keeling (2006) and Bousquet
et al. (2005), which is strongly affected by large-scale wild
fi
res
as in 1997 to 1998, by El Niño events and by the Mt. Pinatubo
eruption.
The effect of climate change on tropospheric chemistry
has been investigated in several studies. In most cases, the
future CH
4
lifetime increases when emissions increase and
climate change is ignored (Brasseur et al., 1998; Stevenson
et al., 2000; Hauglustaine and Brasseur, 2001; Prather et al.,
2001; Hauglustaine et al., 2005). This re
fl
ects the fact that
increased levels of CH
4
and CO depress OH, reducing the CH
4
sink. However, climate warming increases the temperature-
dependent CH
4
oxidation rate coef
fi
cient (Johnson et al.,
1999), and increases in water vapour and NO
x
concentrations
tend to increase OH. In most cases, these effects partly offset
or exceed the CH
4
lifetime increase due to emissions. As a
consequence, the future CH
4
lifetime calculated by Brasseur
et al. (1998), Stevenson et al. (2000) and Hauglustaine et al.
553
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
(2005) remains relatively constant (within a few percent) over
the 21st century. In their transient simulation over the period
1990 to 2100, Johnson et al. (2001)
fi
nd a dominant effect of
climate change on OH in the free troposphere so that the global
CH
4
lifetime declines from about 9 years in 1990 to about 8.3
years by 2025 but does not change signi
fi
cantly thereafter.
Hence the evolution of the CH
4
lifetime depends on the
relative timing of NO
x
and hydrocarbon emission changes in
the emission scenarios, causing the calculated CH
4
increase in
2100 to be reduced by 27% when climate change is considered.
Stevenson et al. (2006) reach a similar conclusion about the
relatively constant CH
4
lifetime. As a result of future changes
in emissions, the CH
4
steady-state lifetime simulated by 25
state-of-the-art CTMs increases by 2.7 ± 2.3% in 2030 from an
ensemble mean of 8.7 ± 1.3 years for the present day (mean ±
1 standard deviation) for a current legislation scenario of future
emissions of ozone precursors. Under the 2030 warmer climate
scenario, the lifetime is reduced by 4.0 ± 1.8%: the total effect
of both emission and climate changes reduces the CH
4
lifetime
by only 1.3%.
7.4.6
Stratospheric Ozone and Climate
From about 1980 to the mid-1990s a negative trend in
globally averaged total ozone occurred, due primarily to an
increase in Cl and bromine loading (Montzka et al., 1999). A
reduction in halogen loading appears to have occurred recently
(Montzka et al., 2003) as well as the beginning of ozone
recovery (e.g., Newchurch et al., 2003; Huck et al., 2005;
Reinsel et al., 2005; Yang et al., 2005). Evidence suggests that a
sustainable recovery of ozone is not expected before the end of
the current decade (e.g., Steinbrecht et al., 2004; Dameris et al.,
2006). Atmospheric concentrations of LLGHGs have increased
(see Chapter 2) and are expected to continue to increase,
with consequences for the ozone layer. This section assesses
current understanding of interactions and feedbacks between
stratospheric ozone and climate. More detailed discussions can
be found in recent reports (European Commission, 2003; IPCC/
TEAP, 2005).
7.4.6.1 Interactions
Stratospheric ozone is affected by climate change through
changes in dynamics and in the chemical composition of the
troposphere and stratosphere. An increase in the concentrations
of LLGHGs, especially CO
2
, cools the stratosphere, allowing
the possibility of more PSCs, and alters the ozone distribution
(Rosenlof et al., 2001; Rosen
fi
eld et al., 2002; Randel et al.,
2004, 2006; Fueglistaler and Haynes, 2005). With the possible
exception of the polar lower stratosphere, a decrease in
temperature reduces ozone depletion leading to higher ozone
column amounts and a positive correction to the LLGHG-
induced radiative cooling of the stratosphere. Moreover, ozone
itself is a greenhouse gas and absorbs UV radiation in the
stratosphere. Absorption of UV radiation provides the heating
responsible for the observed temperature increase with height
above the tropopause. Changes in stratospheric temperatures,
induced by changes in ozone or LLGHG concentration, alter
the Brewer-Dobson circulation (Butchart and Scaife, 2001;
Butchart et al., 2006), controlling the rate at which long-lived
molecules, such as LLGHGs, CFCs, HCFCs and halogens
are transported from the troposphere to various levels in the
stratosphere
.
Furthermore, increases in the Brewer-Dobson
circulation increase temperatures adiabatically in the polar
regions and decrease temperatures adiabatically in the tropics.
Climate is affected by changes in stratospheric ozone,
which radiates infrared radiation down to the troposphere. For
a given percentage change in the vertical structure of ozone,
the largest dependence of the radiative forcing is in the upper
troposphere and ozone layer regions (e.g., TAR, Figure 6.1).
Past ozone depletion has induced surface cooling (Chapter 2).
The observed decrease in stratospheric ozone and the resultant
increase in UV irradiance (e.g., Zerefos et al., 1998; McKenzie
et al., 1999) have affected the biosphere and biogenic emissions
(Larsen, 2005). Such UV radiation increases lead to an enhanced
OH production, reducing the lifetime of CH
4
and in
fl
uencing
tropospheric ozone, both important greenhouse gases (European
Commission, 2003). In addition to global mean equilibrium
surface temperature changes, local surface temperature changes
have been identi
fi
ed by Gillett and Thompson (2003) as a result
of ozone loss from the lower stratosphere. Observational (e.g.,
Baldwin and Dunkerton, 1999, 2001; Thompson et al., 2005)
and modelling (Polvani and Kushner, 2002; Norton, 2003;
Song and Robinson, 2004; Thompson et al., 2005) evidence
exists for month-to-month changes to the stratospheric
fl
ow
feedback to the troposphere, affecting its circulation. Model
results show that trends in the SH stratosphere can affect high-
latitude surface climate (Gillett and Thompson, 2003).
7.4.6.2
Past Changes in Stratospheric Ozone
Ozone losses have been largest in the polar lower stratosphere
during later winter and spring. For example, the ozone hole
over Antarctica has occurred every spring since the early 1980s
(Fioletov et al., 2002). Antarctic ozone destruction is driven by
climatologically low temperatures combined with high Cl and
bromine amounts produced from photochemical breakdown
of primarily anthropogenic CFCs and halons. Similar losses,
smaller in magnitude, have occurred over the Arctic due to
the same processes during cold winters. During warm winters,
arctic ozone has been relatively unaffected (Tilmes et al.,
2004). The antarctic lower stratosphere is nearly always cold
enough to produce substantial ozone loss, but in the year 2002,
a sudden stratospheric warming split the early ozone hole into
two separate regions (e.g., Simmons et al., 2005). Temperatures
were subsequently too high to produce further ozone loss.
Following the later merging of the two separate regions back
into a single vortex, the dynamical conditions were unsuitable
for further ozone loss. This is not an indication of recovery in
ozone amounts, but rather the result of a dynamical disturbance
(e.g., Newman et al., 2004). A summary of recent stratospheric
ozone changes is given in Chapter 2.
554
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.4.6.3
Future Changes in Stratospheric Ozone
The evolution of stratospheric ozone over the next few
decades will depend on natural, including solar and volcanic
activity (e.g., Steinbrecht et al., 2004; Dameris et al., 2005), and
human-caused factors such as stratospheric halogen loading,
which is expected to decrease over future decades (WMO, 2003;
IPCC/TEAP, 2005). The evolution of ozone will also depend on
changes in many stratospheric constituents: it is expected that
the reduction of ozone-depleting substances in the 21st century
will cause ozone to increase via chemical processes (Austin et
al., 2003). However, this increase could be strongly affected by
temperature changes (due to LLGHGs), other chemical changes
(e.g., due to water vapour) and transport changes. Coupled
Chemistry-Climate Models (CCMs) provide tools to simulate
future atmospheric composition and climate. For this purpose,
a set of consistent model forcings has been prescribed as part
of the CCM Validation Activity for Stratospheric Processes and
their Role in Climate (SPARC CCMVal; Eyring et al., 2005).
Forcings include natural and anthropogenic emissions based on
existing scenarios, atmospheric observations and the Kyoto and
Montreal Protocols and Amendments. The simulations follow
the IPCC SRES scenario A1B (IPCC, 2000) and changes
in halocarbons as prescribed in Table 4B-2 of WMO (2003).
Figure 7.18 shows the late winter minimum total column
ozone poleward of 60° for various transient CCM reference
simulations compared with observations. Antarctic ozone
follows mainly the behaviour of Cl and bromine in the models.
The peak depletion simulated by the CCMs occurs around
the year 2000 followed by a slow increase with minimum
values remaining constant between 2000 and 2010 in many
models. Most models predict that antarctic ozone amounts
will increase to 1980 values close to the time when modelled
halogen amounts decrease to 1980 values, lagging the recovery
in mid-latitudes due to the delay associated with transport of
stratospheric air to polar regions. The late return to pre-1980
values by about 2065 in the Atmospheric Model with Transport
and Chemistry (AMTRAC) model (Austin and Wilson, 2006) is
consistent with an empirical model study based on observations
(Newman et al., 2006). Moreover, increased atmospheric
fl
uxes
of CFCs have recently been reported (Hurst et al., 2006), which
may point to a still later recovery. The CCMs do not predict
consistent values for minimum arctic column ozone, with some
models showing large discrepancies with observations. In all
CCMs that have been run long enough, arctic ozone increases
to 1980 values before antarctic ozone does, by as much as 30
years (e.g., Austin and Wilson 2006). This delay in the Antarctic
arises from an increased Brewer-Dobson circulation (Butchart
and Scaife, 2001; Butchart et al., 2006) combined with a
reduction in stratospheric temperatures.
Figure 7.18.
(a) Minimum arctic total column ozone for March to April and (b)
minimum antarctic total column ozone for September to October (both poleward of
60°) in Dobson Units (DU). Simulations of future evolution of ozone were performed
by 11 CCMs analysed as part of the CCM Validation Activity for SPARC (http://www.
pa.op.dlr.de/CCMVal/). Model results are compared with values calculated from
the National Institute of Water and Atmospheric Research (NIWA) assimilated total
column ozone database shown as black dots (Bodeker et al., 2005). The light grey
shading between 2060 and 2070 shows the period when halogen amounts in the
polar lower stratosphere are expected to return to 1980 values. Models include
AMTRAC: Atmospheric Model with Transport and Chemistry; CCSRNIES: Center for
Climate System Research - National Institute for Environmental Studies; CMAM:
Canadian Middle Atmosphere Model; E39C: German Aerospace Center (DLR) version
of ECHAM4 with chemistry and 39 levels; GEOSCCM: Goddard Earth Observing
System Chemistry-Climate Model; MAECHAM4/CHEM: Middle Atmosphere ECHAM4
with Chemistry; MRI: Meteorological Research Institute; SOCOL: Solar Climate Ozone
Links; ULAQ: University of L’Aquila; UMSLIMCAT: Unifi ed Model SLIMCAT; WACCM:
Whole Atmosphere Community Climate Model.
555
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.4.6.4 Uncertainties Due to Atmospheric Dynamics
Changes in atmospheric dynamics could affect ozone.
For example, sub-grid scale processes such as gravity wave
propagation (e.g., Warner and McIntyre, 2001), prescribed
for past and present conditions, may change in the future.
Tropospheric climate changes will also alter planetary-scale
waves. Together with changes in orographic gravity waves, these
waves give rise to the increase in the Brewer-Dobson circulation
seen in most models (Butchart et al., 2006). The magnitude of
this effect varies from model to model and leads to increased
adiabatic heating of the polar regions, compensating in part the
increased radiative cooling from CO
2
increases. Hence, the net
heating or cooling is subject to large uncertainty, and available
model simulations do not give a consistent picture of future
development of ozone, particularly in the Arctic (Figure 7.18).
7.5
Aerosol Particles and the Climate
System
Aerosols are an integral part of the atmospheric hydrological
cycle and the atmosphere’s radiation budget, with many possible
feedback mechanisms that are not yet fully understood. This
section assesses (1) the impact of meteorological (climatic)
factors like wind, temperature and precipitation on the natural
aerosol burden and (2) possible effects of aerosols on climate
parameters and biogeochemistry. The most easily understood
interaction between aerosols and climate is the direct effect
(scattering and absorption of shortwave and thermal radiation),
which is discussed in detail in Chapter 2. Interactions with the
hydrological cycle, and additional impacts on the radiation
budget, occur through the role of aerosols in cloud microphysical
processes, as aerosol particles act as cloud condensation nuclei
(CCN) and ice nuclei (IN). The suite of possible impacts of
aerosols through the modi
fi
cation of cloud properties is called
‘indirect effects’. The forcing aspect of the indirect effect at
the top of the atmosphere is discussed in Chapter 2, while the
processes that involve feedbacks or interactions, like the ‘cloud
lifetime effect’
6
, the ‘semi-direct effect’ and aerosol impacts on
the large-scale circulation, convection, the biosphere through
nutrient supply and the carbon cycle, are discussed here.
7.5.1
Aerosol Emissions and Burdens Affected by
Climatic Factors
Most natural aerosol sources are controlled by climatic
parameters like wind, moisture and temperature. Hence, human-
induced climate change is also expected to affect the natural
aerosol burden. The sections below give a systematic overview
of the major natural aerosol sources and their relations to
climate parameters while anthropogenic aerosol emissions and
combined aerosols are the subject of Chapter 2.
7.5.1.1 Dust
Estimates of the global source strength of bulk dust aerosols
with diameters below 10
μ
m of between 1,000 and 3,000
Tg yr
–1
agree well with a wide range of observations (Duce,
1995; Textor et al., 2005; Cakmur et al., 2006). Seven to twenty
percent of the dust emissions are less than 1
μ
m in diameter
(Cakmur et al., 2006; Schulz et al., 1998). Zhang et al. (1997)
estimated that about 800 Tg yr
–1
of Asian dust emissions are
injected into the atmosphere annually, about 30% of which is re-
deposited onto the deserts and 20% is transported over regional
scales, while the remaining approximately 50% is subject to
long-range transport to the Paci
fi
c Ocean and beyond. Asian dust
appears to be a continuous source that dominates background
dust aerosol concentrations on the west coast of the USA (Duce,
1995; Perry et al., 2004). Uncertainties in the estimates of global
dust emissions are greater than a factor of two (Zender et al.,
2004) due to problems in validating and modelling the global
emissions. The representation of the high wind tail of the wind
speed distribution alone, responsible for most of the dust
fl
ux,
leads to differences in emissions of more then 30% (Timmreck
and Schulz, 2004). Observations suggest that annual mean
African dust may have varied by a factor of four during 1960
to 2000 (Prospero and Lamb, 2003), possibly due to rainfall
variability in the Sahel zone. Likewise, simulations of dust
emissions in 2100 are highly uncertain, ranging from a 60%
decrease to a factor of 3.8 increase as compared to present-day
dust emissions (Mahowald and Luo, 2003; Tegen et al., 2004;
Woodward et al., 2005; Stier et al., 2006a). Reasons for these
discrepancies include different treatments of climate-biosphere
interactions and the climate model used to drive the vegetation
and dust models. The potentially large impact of climate change
on dust emissions shows up in particular when comparing
present-day with LGM conditions for dust erosion (e.g., Werner
et al., 2002).
The radiative effect of dust, which, for example, could
intensify the African Easterly Waves, may be a feedback
mechanism between climate and dust (Jones et al., 2004). It
also alters the atmospheric circulation, which feeds back to
dust emission from natural sources (see Section 7.5.4). Perlwitz
et al. (2001) estimate that this feedback reduces the global
dust load by roughly 15%, as dust radiative forcing reduces
the downward mixing of momentum within the planetary
boundary layer, the surface wind speed, and thus dust emission
(Miller et al., 2004a). In addition to natural dust production,
human activities have created another potential source for
dust mobilisation through deserti
fi
cation. The contribution
to global dust emission of deserti
fi
cation through human
activities is uncertain: estimates vary from 50% (Tegen et al.,
1996; Mahowald et al., 2004) to less than 10% (Tegen et al.,
2004) to insigni
fi
cant values (Ginoux et al., 2001; Prospero et
al., 2002). A 43-year estimate of Asian dust emissions reveals
that meteorology and climate have a greater in
fl
uence on Asian
6
The processes involved are more complex than can be encompassed in a single expression. The term ‘cloud lifetime effect’ thus should be understood to mean that aerosols can
change precipitation effi ciency in addition to increasing cloud albedo.
556
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
dust emissions and associated Asian dust storm
occurrences than does deserti
fi
cation (Figure
7.19; Zhang et al., 2003).
In addition, aerosol deposition affects global
ecosystems. Deposition of mineral dust plays an
important role in the biogeochemical cycle of the
oceans, by providing the nutrient iron, which affects
ocean biogeochemistry with feedbacks to climate
and dust production (Jickells et al., 2005; Section
7.3.4.4). Conversely, water-soluble particulate
iron over the Paci
fi
c Ocean is linked to elemental
carbon emissions resulting from anthropogenic
activity in Asia (Chuang et al., 2005). The input
of trace elements by dust deposition is also of
importance to terrestrial ecosystems. For example,
it has been proposed that the vegetation of the
Amazon basin is highly dependent on Saharan dust
deposition, which provides phosphorus, necessary
for maintenance of long-term productivity (Okin
et al., 2004; Section 7.3). The Hawaiian Islands
also depend on phosphorus from Asian dust
transport (Chadwick et al., 1999). Moreover,
mineral dust can act as a sink for acidic trace
gases, such as sulphur dioxide (SO
2
) and HNO
3
,
and thereby interact with the sulphur and N cycles
(e.g., Dentener et al., 1996; Umann et al., 2005).
Coatings with soluble substances, such as sulphate
or nitrate, will change the ability of mineral dust
aerosols to nucleate cloud droplets (Levin et al.,
1996; Section 7.5.2.1).
7.5.1.2 Sea
Salt
Sea salt aerosol is a key aerosol constituent of
the marine atmosphere. Sea salt aerosol particles
affect the formation of clouds and rain. They serve
as sinks for reactive gases and small particles and
possibly suppress new particle formation. Sea
salt is also responsible for a large fraction of the non-sea salt
sulphate formation (e.g., Sievering et al., 1992). The major
meteorological and environmental factors that affect sea salt
formation are wind speed, atmospheric stability and wind
friction velocity, sea surface and air temperatures, present and
prior rain or snow and the amount and nature of surface-active
materials in the near-surface ocean waters (Lewis and Schwartz,
2005). The average annual global sea salt
fl
ux from 12 models
is estimated to be 16,300 Tg ± 200% (Textor et al., 2005) of
which 15% is emitted into the submicron mode.
7.5.1.3
Natural Organic Carbon
Biogenic organic material is both directly emitted into the
atmosphere and produced by VOCs. Primary emissions from the
continents have been thought to be a relatively minor source but
some studies suggest that these emissions could be much higher
than previously estimated (Folberth et al., 2005; Jaenicke, 2005).
Kanakidou et al. (2005) estimate a global biogenic secondary
organic aerosol production of about 30 Tg yr
–1
and recognise the
potentially large, but uncertain,
fl
ux of primary biogenic particles.
Annual global biogenic VOC emission estimates range from 500
to 1,200 Tg yr
–1
(Guenther et al., 1995). There is a large range
(less than 5 to greater than 90%) of organic aerosol yield for
individual compounds and atmospheric conditions resulting in
estimates of global annual secondary organic aerosol production
from biogenic VOCs that range from 2.5 to 44.5 Tg of organic
matter per year (Tsigaridis and Kanakidou, 2003). All biogenic
VOC emissions are highly sensitive to changes in temperature,
and some emissions respond to changes in solar radiation and
precipitation (Guenther et al., 1995). In addition to the direct
response to climatic changes, biogenic VOC emissions are also
highly sensitive to climate-induced changes in plant species
composition and biomass distributions.
Figure 7.19.
(a) Chinese desert distributions from 1960 to 1979 and desert plus desertifi cation
areas from 1980 to 1999. (b) Sources (S1 to S10) and typical depositional areas (D1 and D2) for
Asian dust indicated by spring average dust emission fl ux (kg km
–2
per month) averaged over 1960
to 2002. The percentages with standard deviations in parentheses denote the average amount of
dust production in each source region and the total amount of emissions between 1960 and 2002.
The deserts in Mongolia (S2) and in western (S4) and northern (S6) China (mainly the Taklimakan
and Badain Juran, respectively) can be considered the major sources of Asian dust emissions.
Several areas with more expansions of deserts (S7, S8, S9 and S5) are not key sources. Adapted
from Zhang et al. (2003).
557
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Global biogenic VOC emissions respond to climate change
(e.g., Turner et al., 1991; Adams et al., 2001; Penner et al.,
2001; Sanderson et al., 2003b). These model studies predict
that solar radiation and climate-induced vegetation change can
affect emissions, but they do not agree on the sign of the change.
Emissions are predicted to increase by 10% per °C
(Guenther et
al., 1993). There is evidence of physiological adaptation to higher
temperatures that would lead to a greater response for long-
term temperature changes (Guenther et al., 1999). The response
of biogenic secondary organic carbon aerosol production to a
temperature change, however, could be considerably lower than
the response of biogenic VOC emissions since aerosol yields can
decrease with increasing temperature. A potentially important
feedback among forest ecosystems, greenhouse gases, aerosols
and climate exists through increased photosynthesis and forest
growth due to increasing temperatures and CO
2
fertilization
(Kulmala et al., 2004). Increased forest biomass would increase
VOC emissions and thereby organic aerosol production. This
couples the climate effect of CO
2
with that of aerosols.
New evidence shows that the ocean also acts as a source
of organic matter from biogenic origin (O’Dowd et al., 2004;
Leck and Bigg, 2005b). O’Dowd et al. (2004) show that during
phytoplankton blooms (summer conditions), the organic
aerosols can constitute up to 63% of the total aerosol. Surface-
active organic matter of biogenic origin (such as lipidic and
proteinaceous material and humic substances), enriched in the
oceanic surface layer and transferred to the atmosphere by bubble-
bursting processes, are the most likely candidates to contribute
to the observed organic fraction in marine aerosol. Insoluble
heat-resistant organic sub-micrometre particles (peaking at 40 to
50 nm in diameter), mostly combined into chains or aggregated
balls of ‘marine microcolloids’ linked by an amorphous electron-
transparent material with properties entirely consistent with
exopolymer secretions (Decho, 1990; Verdugo et al., 2004), are
found in near-surface water of lower-latitude oceans (Benner
et al., 1992; Wells and Goldberg, 1994), in leads between ice
fl
oes (Bigg et al., 2004), above the arctic pack ice (Leck and
Bigg, 2005a) and over lower-latitude oceans (Leck and Bigg,
2005b). This aerosol formation pathway may constitute an ice
(microorganisms)-ocean-aerosol-cloud feedback.
7.5.1.4
Aerosols from Dimethyl Sulphide
Dimethyl sulphide produced by phytoplankton is the most
abundant form in which the ocean releases gaseous sulphur.
Sea-air
fl
uxes of DMS vary by orders of magnitude depending
mainly on DMS sea surface concentration and on wind speed.
Estimates of the global DMS
fl
ux vary widely depending
mainly on the DMS sea surface climatology utilised, sea-air
exchange parametrization and wind speed data, and range from
16 to 54 Tg yr
–1
of sulphur (see Kettle and Andreae, 2000 for
a review). According to model studies (Gondwe et al., 2003;
Kloster et al., 2006), 18 to 27% of the DMS is converted into
sulphate aerosols. Penner et al. (2001) show a small increase
in DMS emissions between 2000 and 2100 (from 26.0 to 27.7
Tg yr
–1
of sulphur) using constant DMS sea surface
concentrations together with a constant monthly climatological
ice cover. Gabric et al. (2004) predict an increase of the globally
integrated DMS
fl
ux perturbation of 14% for a tripling of the
pre-industrial atmospheric CO
2
concentration.
Bopp et al. (2004) estimate the feedback of DMS to cloud
albedo with a coupled atmosphere-ocean-biogeochemical
climate model that includes phytoplankton species in the ocean
and a sulphur cycle in the atmospheric climate model. They
obtain an increase in the sea-air DMS
fl
ux of 3% for doubled
atmospheric CO
2
conditions, with large spatial heterogeneities
(–15 to +30%). The mechanisms affecting those
fl
uxes are
marine biology, relative abundance of phytoplankton types
and wind intensity. The simulated increase in
fl
uxes causes
an increase in sulphate aerosols and, hence, cloud droplets
resulting in a radiative perturbation of cloud albedo of –0.05
W m
–2
, which represents a small negative climate feedback to
global warming.
7.5.1.5
Aerosols from Iodine Compounds
Intense new aerosol particle formation has been frequently
observed in the coastal environment (O’Dowd et al., 2002a).
Simultaneous coastal observations of reactive iodine species
(Saiz-Lopez et al., 2005), chamber studies using iodocarbon
precursors and laboratory characterisation of iodine oxide
particles formed from exposure of
Laminaria
macroalgae to
ozone (McFiggans et al., 2004) have demonstrated that coastal
particle formation is linked to iodine compound precursor
released from abundant infralittoral beds of macroalgae. The
particle bursts overwhelmingly occur during daytime low tides
(O’Dowd et al., 2002b; Saiz-Lopez et al., 2005). Tidal exposure
of kelp leads to the well-documented release of signi
fi
cant
fl
uxes
of iodocarbons (Carpenter et al., 2003), the most photolabile of
which, di-iodomethane (CH
2
I
2
), may yield a high iodine atom
fl
ux. However, the iodine monoxide (IO) and iodine dioxide
(OIO) radicals, and new particles are thought more likely to
result from emissions of molecular iodine (McFiggans et al.,
2004), which will yield a much greater iodine atom
fl
ux (Saiz-
Lopez and Plane, 2004). It is unclear whether such particles
grow suf
fi
ciently to act as CCN (O’Dowd, 2002; Saiz-Lopez et
al., 2005). Thus, a hitherto undiscovered remote ocean source
of iodine atoms (such as molecular iodine) must be present if
iodine-mediated particle formation is to be important in the
remote marine boundary layer (McFiggans, 2005).
7.5.1.6
Climatic Factors Controlling Aerosol Burdens
and Cycling
As discussed above, near-surface wind speed determines
the source strength for primary aerosols (sea salt, dust, primary
organic particles) and precursors of secondary aerosols (mainly
DMS). Progress has been made in the development of source
functions (in terms of wind speed) for sea salt and desert dust
(e.g., Tegen et al., 2002; Gong, 2003; Balkanski et al., 2004).
558
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Wind speed also affects dry deposition velocities and hence the
lifetime of aerosols. In addition, biogenic emissions are strongly
dependent on temperature (together with humidity/moisture;
e.g., Guenther et al., 1995). Temperature also is a key factor in
the gas-aerosol partitioning of semi-volatile secondary organics
(Kanakidou et al., 2005).
Precipitation directly affects the wet removal and hence
the lifetime of atmospheric aerosols. More aerosols decrease
the precipitation formation rate, which in turn increases the
lifetime of aerosols and results in more long-range aerosol
transport to remote regions where wet removal is less ef
fi
cient.
At the same time, precipitating boundary layer clouds maintain
themselves by keeping aerosol concentrations low (e.g., Baker
and Charlson, 1990; Stevens et al., 2005; Sharon et al., 2006).
Precipitation also affects soil moisture, with impacts on dust
source strength and on stomatal opening/closure of plant
leaves, hence affecting biogenic emissions. Cloud processing
is an important pathway in the gas-to-particle conversion. It
is the most important oxidation pathway for sulphate aerosols
and shifts the aerosol size distribution to larger sizes, such that
aerosols are more easily activated in subsequent cloud events
(e.g., Hoppel et al., 1990; Kerkweg et al., 2003; Yin et al.,
2005). It is also important in the conversion of hydrophobic to
hydrophilic carbon.
Aerosol burden and lifetime are also affected by
microphysical interactions among the different aerosol
compounds as well as by changes in the spatial and seasonal
distribution of the emissions. Sea salt aerosols, for example,
provide surfaces for conversion of SO
2
into sulphate aerosols
(Sievering et al., 1992) with consequences for cloud formation
(Gong and Barrie, 2003; Section 7.5.2.1). A future reduction
in SO
2
emissions and the associated reduced conversion of
hydrophobic to hydrophilic soot could lead to a prolonged
residence time of soot (Cooke et al., 2002; Stier et al., 2006b)
and increased ammonium nitrate (Liao and Seinfeld, 2005).
However, in a transient AOGCM climate simulation with an em-
bedded microphysical aerosol module, Stier et al. (2006a) show
that the effect on the hydrophobic to hydrophilic conversion
can be outweighed by a general shift to low-latitude dry-season
soot emissions. Consequently, soot lifetime increases in a future
climate despite an enhanced conversion of hydrophobic to
hydrophilic soot.
Table 7.10a.
Overview of the different aerosol indirect effects and their sign of the net radiative fl ux change at the top of the atmosphere (TOA).
Effect
Cloud Types
Affected
Process
Sign of Change
in TOA Radiation
Potential
Magnitude
Scientifi c
Understanding
Cloud albedo effect
All clouds
For the same cloud water or ice content
more but smaller cloud particles refl ect
more solar radiation
Negative Medium
Low
Cloud lifetime effect
All clouds
Smaller cloud particles decrease
the precipitation effi ciency thereby
presumably prolonging cloud lifetime
Negative
Medium
Very low
Semi-direct effect
All clouds
Absorption of solar radiation by absorbing
aerosols affects static stability and the
surface energy budget, and may lead to
an evaporation of cloud particles
Positive or
negative
Small
Very low
Glaciation indirect effect
Mixed-phase
clouds
An increase in IN increases the
precipitation effi ciency
Positive
Medium
Very low
Thermodynamic effect
Mixed-phase
clouds
Smaller cloud droplets delay freezing
causing super-cooled clouds to extend to
colder temperatures
Positive or
negative
Medium
Very low
Table 7.10b.
Overview of the different aerosol indirect effects and their implications for the global mean net shortwave radiation at the surface, F
sfc
(Columns 2-4) and for
precipitation (Columns 5-7).
Effect
Sign of Change
in F
sfc
Potential
Magnitude
Scientifi c
Understanding
Sign of Change
in Precipitation
Potential
Magnitude
Scientifi c
Understanding
Cloud albedo effect
Negative
Medium
Low
n.a.
n.a.
n.a.
Cloud lifetime effect
Negative
Medium
Very low
Negative
Small
Very low
Semi-direct effect
Negative
Large
Very low
Negative
Large
Very low
Glaciation indirect effect
Positive
Medium
Very low
Positive
Medium
Very low
Thermodynamic effect
Positive or
negative
Medium
Very low
Positive or
negative
Medium
Very low
559
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
7.5.2
Indirect Effects of
Aerosols on Clouds
and Precipitation
Aerosols can interact with clouds
and precipitation in many ways,
acting either as CCN or IN, or as
absorbing particles, redistributing
solar energy as thermal energy
inside cloud layers. These indirect
effects (in contrast to the direct
interaction with radiation, see
Chapter 2) are the subject of this
subsection. They can be subdivided
into different contributing processes,
as summarised in Table 7.10 and
shown in Figure 7.20. Cloud
feedbacks remain the largest source
of uncertainty in climate sensitivity
estimates and the relatively poor
simulation of boundary layer clouds
in the present climate is a reason
for some concern (see Chapter 8).
Therefore the results discussed
below need to be considered with
caution.
The cloud-albedo effect, that
is, the distribution of the same
cloud liquid water content over
more, hence smaller, cloud droplets
leading to higher cloud re
fl
ectivity,
is a purely radiative forcing and is
therefore treated in Chapter 2. The
other effects involve feedbacks in
the climate system and are discussed
here. The albedo effect cannot be
easily separated from the other
effects; in fact, the processes that
decrease the cloud droplet size per
given liquid water content also
decrease precipitation formation,
presumably prolonging cloud
lifetime (cloud lifetime effect,
Section 7.5.2.1 and Figure 7.20). In
turn, an increase in cloud lifetime
also contributes to a change in the
time-averaged cloud albedo. The
semi-direct effect refers to the absorption of solar radiation
by soot, re-emitted as thermal radiation, hence heating the air
mass and increasing static stability relative to the surface. It
may also cause evaporation of cloud droplets (see Sections 2.4
and 7.5.4.1 and Figure 7.20). The glaciation effect refers to an
increase in IN resulting in a rapid glaciation of a super-cooled
liquid water cloud due to the difference in vapour pressure over
ice and water. Unlike cloud droplets, these ice crystals grow
in an environment of high super-saturation with respect to ice,
quickly reaching precipitation size, with the potential to turn
a non-precipitating cloud into a precipitating cloud (Section
7.5.2.2 and Figure 7.20). The thermodynamic effect refers to a
delay in freezing by the smaller droplets causing super-cooled
clouds to extend to colder temperatures (Section 7.5.2.2 and
Figure 7.20). In addition to aerosol-induced changes at the top
of the atmosphere (TOA), aerosols affect the surface energy
budget (Table 7.10b; Section 7.5.2) with consequences for
convection, evaporation and precipitation (Figure 7.20).
Figure 7.20.
Schematic diagram of the aerosol effects discussed in Table 7.10. TOA refers to the top-of-the-atmosphere.
560
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.5.2.1
Aerosol Effects on Water Clouds and Warm
Precipitation
Aerosols are hypothesised to increase the lifetime of clouds
because increased concentrations of smaller droplets lead
to decreased drizzle production and reduced precipitation
ef
fi
ciency (Albrecht,
1989). It is dif
fi
cult to devise
observational studies that can separate the cloud lifetime from
the cloud albedo effect (see Section 2.4). Thus, observational
studies usually provide estimates of the combined effects.
Similarly, climate models cannot easily separate the cloud
lifetime indirect effect once the aerosol scheme is fully coupled
to a cloud microphysics scheme, but also predict the combined
cloud albedo, lifetime and semi-direct effect.
Evidence for the absence of a drizzle mode due to
anthropogenic emissions of aerosols and their precursors
comes, for instance, from ship tracks perturbing marine stratus
cloud decks off the coast of California (Ferek et al., 1998) as
well as from analysing polluted compared with clean clouds off
the Atlantic coast of Canada (Peng et al., 2002). One problem
is that most climate models suggest an increase in liquid water
when adding anthropogenic aerosols, whereas newer ship track
studies show that polluted marine water clouds can have less
liquid water than clean clouds (Platnick et al., 2000; Coakley
and Walsh, 2002). Ackerman et al. (2004) attribute this effect
to enhanced entrainment of dry air in polluted clouds in these
instances with subsequent evaporation of cloud droplets.
Similarly, when cloud lifetime is analysed, an increase in
aerosol concentration from very clean to very polluted does not
increase cloud lifetime, even though precipitation is suppressed
(Jiang et al., 2006). This effect is due to competition between
precipitation suppression and enhanced evaporation of the more
numerous smaller cloud droplets in polluted clouds. Observed
lower aerosol concentrations in pockets of open cells (Stevens et
al., 2005) and in rifts of broken clouds surrounded by solid decks
of stratocumulus with higher aerosol concentrations (Sharon
et al., 2006) are manifestations of two stable aerosol regimes
(Baker and Charlson, 1990). The low aerosol concentration
regimes maintain themselves by higher drizzle rates. However,
it is hard to disentangle cause and effect from these studies.
Smoke from burning vegetation reduces cloud droplet sizes
and delays the onset of precipitation (Warner and Twomey, 1967;
Rosenfeld, 1999; Andreae et al., 2004). In addition, desert dust
suppresses precipitation in thin low-altitude clouds (Rosenfeld
et al., 2001; Mahowald and Kiehl, 2003). Contradictory results
have been found regarding the suppression of precipitation
by aerosols downwind of urban areas (Givati and Rosenfeld,
2004; Jin et al., 2005) and in Australia (Rosenfeld, 2000; Ayers,
2005).
Models suggest that anthropogenic aerosols suppress
precipitation in the absence of giant CCN and aerosol-induced
changes in ice microphysics (e.g., Lohmann, 2002; Menon and
DelGenio, 2007) as well as in mixed-phase clouds where the ice
phase only plays a minor role (Phillips et al., 2002). A reduction
in precipitation formation leads to increased cloud processing
of aerosols. Feingold et al. (1998) and Wurzler et al. (2000)
showed that cloud processing could either lead to an increase or
decrease in precipitation formation in subsequent cloud cycles,
depending on the size and concentration of activated CCN. Giant
sea salt nuclei, on the other hand, may override the precipitation
suppression effect of the large number of small pollution
nuclei (Johnson, 1982; Feingold et al., 1999; Rosenfeld et al.,
2002). Likewise, Gong and Barrie (2003) predict a reduction
of 20 to 60% in marine cloud droplet number concentrations
and an increase in precipitation when interactions of sulphate
with sea salt aerosols are considered. When aerosol effects on
warm convective clouds are included in addition to their effect
on warm stratiform clouds, the overall indirect aerosol effect
and the change in surface precipitation can be larger or smaller
than if just the aerosol effect on stratiform clouds is considered
(Nober et al., 2003; Menon and Rotstayn, 2006). Besides
changes in the distribution of precipitation, the frequency of
extreme events may also be reduced by the presence of aerosols
(Paeth and Feichter, 2006).
Observations show that aerosols can decrease or increase
cloud cover. Kaufman
et al. (2005) conclude from satellite
observations that the aerosol indirect effect is likely primarily
due to an increase in cloud cover, rather than an increase in
cloud albedo. In contrast, model results of Lohmann et al. (2006)
associate the increase in cloud cover with differing dynamic
regimes and higher relative humidities that maintain higher
aerosol optical depths. On the other hand, the semi-direct effect
of absorbing aerosols can cause evaporation of cloud droplets
and/or inhibit cloud formation. In a large area with absorbing
biomass-burning aerosol, few low-lying clouds were observed
when the aerosol optical depth exceeded 1.2 (Koren et al., 2004).
Increasing emissions of absorbing aerosols from the late 1980s
to the late 1990s in China also reduced cloud amount leading to
a decrease in local planetary albedo, as deduced from satellite
data (Krüger and Grassl, 2004). When the combined effect of
pollution and smoke aerosols is considered from ground-based
observations, the net effect seems to be an increase in cloud
cover with increasing aerosol column concentrations (Kaufman
and Koren, 2006).
7.5.2.2
Aerosol Impacts on Mixed-Phase Clouds
As satellite observations of aerosol effects on mixed-phase
clouds are not conclusive (Mahowald and Kiehl, 2003), this
section only refers to model results and
fi
eld studies. Studies with
GCMs suggest that if, in addition to mineral dust, hydrophilic
black carbon aerosols are assumed to act as IN at temperatures
between 0°C and –35°C, then increases in aerosol concentration
from pre-industrial to present times may cause a glaciation
indirect effect (Lohmann, 2002). Increases in IN can result in
more frequent glaciation of super-cooled stratiform clouds and
increase the amount of precipitation via the ice phase, which
could decrease the global mean cloud cover leading to more
absorption of solar radiation. Whether the glaciation effect or
warm cloud lifetime effect is larger depends on the chemical
561
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
nature of the dust (Lohmann and Diehl, 2006). Likewise, the
number and size of ice particles in convective mixed-phase
clouds is sensitive to the chemical composition of the insoluble
fraction (e.g., dust, soot, biological particles) of the aerosol
particles (Diehl and Wurzler, 2004).
Rosenfeld (1999) and Rosenfeld and Woodley (2000)
analysed aircraft data together with satellite data suggesting
that pollution aerosols suppress deep convective precipitation
by decreasing cloud droplet size and delaying the onset of
freezing. This hypothesis was supported by a cloud-resolving
model study (Khain et al., 2001) showing that super-cooled
cloud droplets down to –37.5°C could only be simulated if the
cloud droplets were small and numerous. Precipitation from
single-cell mixed-phase convective clouds is reduced under
continental and maritime conditions when aerosol concentrations
are increased (Yin et al., 2000; Khain et al., 2004; Seifert and
Beheng, 2006). In the modelling study by Cui et al. (2006), this
is caused by drops evaporating more rapidly in the high aerosol
case (see also Jiang et al., 2006), which eventually reduces ice
mass and hence precipitation. Khain et al. (2005) postulate that
smaller cloud droplets, such as those originating from human
activity, would change the thermodynamics of convective
clouds. More, smaller droplets would reduce the production
of rain in convective clouds. When these droplets freeze, the
associated latent heat release would then result in more vigorous
convection and more precipitation. In a clean cloud, on the other
hand, rain would have depleted the cloud so that less latent heat
is released when the cloud glaciates, resulting in less vigorous
convection and less precipitation. Similar results were obtained
by Koren et al. (2005), Zhang et al. (2005) and for the multi-
cell cloud systems studied by Seifert and Beheng (2006). For
a thunderstorm in Florida in the presence of Saharan dust, the
simulated precipitation enhancement only lasted two hours after
which precipitation decreased as compared with clean conditions
(van den Heever et al., 2006). Cloud processing of dust particles,
sulphate particles and trace gases can lead to an acceleration
of precipitation formation in continental mixed-phase clouds,
whereas in maritime clouds, which already form on rather large
CCN, the simulated effect on precipitation is small (Yin et al.,
2002). This highlights the complexity of the system and indicates
that the sign of the global change in precipitation due to aerosols
is not yet known. Note that microphysical processes can only
change the temporal and spatial distribution of precipitation
while the total amount of precipitation can only change if
evaporation from the surface changes.
7.5.2.3
Aerosol Impacts on Cirrus Clouds
Cirrus clouds can form by homogeneous and heterogeneous
ice nucleation mechanisms at temperatures below 235 K.
While homogeneous freezing of super-cooled aqueous phase
aerosol particles is rather well understood, understanding of
heterogeneous ice nucleation is still in its infancy. A change in the
number of ice crystals in cirrus clouds could exert a cloud albedo
effect in the same way that the cloud albedo effect acts for water
clouds. In addition, a change in the cloud ice water content could
exert a radiative effect in the infrared. The magnitude of these
effects in the global mean has not yet been fully established, but
the development of physically based parametrization schemes
of cirrus formation for use in global models led to signi
fi
cant
progress in understanding underlying mechanisms of aerosol-
induced cloud modi
fi
cations (Kärcher and Lohmann, 2002; Liu
and Penner, 2005; Kärcher et al., 2006).
A global climate model study concluded that a cloud albedo
effect based solely on ubiquitous homogeneous freezing is
small globally (Lohmann and Kärcher, 2002). This is expected
to also hold in the presence of heterogeneous IN that cause
cloud droplets to freeze at relative humidities over ice close to
homogeneous values (above 130–140%) (Kärcher and Lohmann,
2003). Ef
fi
cient heterogeneous IN, however, would be expected
to lower the relative humidity over ice, so that the climate effect
may be larger (Liu and Penner, 2005).
In situ
measurements
reveal that organic-containing aerosols are less abundant than
sulphate aerosols in ice cloud particles, suggesting that organics
do not freeze preferentially (Cziczo et al., 2004). A model study
explains this
fi
nding by the disparate water uptake of organic
aerosols, and suggests that organics are unlikely to signi
fi
cantly
modify cirrus formation unless they are present in very high
concentrations (compared with sulphate-rich particles) at low
temperatures (Kärcher and Koop, 2004).
With regard to aerosol effects on cirrus clouds, a strong link
has been established between gravity wave induced, mesoscale
variability in vertical velocities and climate forcing by cirrus
(Kärcher and Ström, 2003; Hoyle et al., 2005). Hemispheric-
scale studies of aerosol-cirrus interactions using ensemble
trajectories suggest that changes in upper-tropospheric cooling
rates and ice-forming aerosols in a future climate may induce
changes in cirrus occurrence and optical properties that are
comparable in magnitude with observed decadal trends in
global cirrus cover (Haag and Kärcher, 2004). Optically thin
and sub-visible cirrus are particularly susceptible to IN and
therefore likely affected by anthropogenic activities.
Radiative forcing estimates and observed trends of aviation-
induced cloudiness are discussed in Section 2.6. In terms of
indirect effects of aircraft-induced aerosols on cirrus clouds,
Lohmann and Kärcher (2002) show that the impact of aircraft
sulphur emissions on cirrus properties via homogeneous
freezing is small. The contribution from air traf
fi
c to the global
atmospheric black carbon cycle was assessed by Hendricks et al.
(2004). Assuming that black carbon particles from aviation serve
as ef
fi
cient IN, maximum increases or decreases in ice crystal
number concentrations of more than 40% are simulated in a
climate model study assuming that the ‘background’ (no aviation
impact) cirrus cloud formation is dominated by heterogeneous
or homogeneous nucleation, respectively (Hendricks et al.,
2005). Progress in assessing the impact of aircraft black carbon
on cirrus is hampered by the poor knowledge of natural freezing
modes in cirrus conditions and the inability to describe the full
complexity of cirrus processes in global models.
562
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
7.5.2.4
Global Climate Model Estimates of the Total
Anthropogenic Aerosol Effect
The total anthropogenic aerosol effect as de
fi
ned here
includes estimates of the direct effect, semi-direct effect,
indirect cloud albedo and cloud lifetime effect for warm
clouds from several climate models. The total anthropogenic
aerosol effect is obtained as the difference between a multi-
year simulation with present-day aerosol emissions and a
simulation representative for pre-industrial conditions, where
anthropogenic emissions are turned off. It should be noted
that the representation of the cloud lifetime effect in GCMs is
essentially one of changing the auto-conversion of cloud water
to rainwater.
The global mean total anthropogenic aerosol effect on net
radiation at TOA from pre-industrial times to the present day
is shown in Figure 7.21. Whereas Chapter 2 only considers the
radiative forcing of the cloud albedo effect, here feedbacks are
included in the radiative
fl
ux change. In most simulations shown
in Figures 7.21 to 7.23, the total aerosol effect is restricted to
warm clouds except for the simulations by Jacobson (2006)
and Lohmann and Diehl (2006), who also include aerosol
effects on mixed-phase and ice clouds. The total aerosol effect
ranges from –0.2 W m
–2
in the combined GCM plus satellite
simulations (Quaas et al., 2006) to –2.3 W m
–2
in the simulations
by Ming et al. (2005), with an average forcing of –1.2 W m
–2
.
The total aerosol effect is larger when sulphate aerosols are used
as surrogates for all anthropogenic aerosols than if multiple
Figure 7.21.
Global mean total anthropogenic aerosol effect (direct, semi-direct and indirect cloud albedo and lifetime effects) defi ned as the response in net radiation at TOA
from pre-industrial times to the present day and its contribution over the NH and SH, over oceans and over land, and the ratio over oceans/land. Red bars refer to anthropogenic
sulphate (Easter et al., 2004; Ming et al., 2005
+
), green bars refer to anthropogenic sulphate and black carbon (Kristjánsson, 2002
*,+
), blue bars to anthropogenic sulphate and
organic carbon (Quaas et al., 2004; Rotstayn and Liu, 2005
+
), cyan bars to anthropogenic sulphate and black and organic carbon (Menon and Del Genio, 2005; Takemura et al.,
2005; Johns et al., 2006; Storelvmo et al., 2006), dark purple bars to anthropogenic sulphate and black and organic carbon effects on water and ice clouds (Jacobson, 2006;
Lohmann and Diehl, 2006), teal bars refer to a combination of GCM and satellite results (European Centre for Medium Range Weather Forecasts/Max-Planck Institute for Meteo-
rology Atmospheric GCM (ECHAM) plus Polarisation and Directionality of the Earth’s Refl ectance (POLDER), Lohmann and Lesins, 2002; Laboratoire de Météorologie Dynamique
GCM (LMDZ)/ECHAM plus Moderate Resolution Imaging Spectroradiometer (MODIS), Quaas et al., 2006) and olive bars to the mean and standard deviation from all simulations.
Vertical black lines for individual results refer to ±1 standard deviation in cases of multiple simulations and/or results.
* refers to estimates of the aerosol effect deduced from the shortwave radiative fl ux only
+
refers to estimates solely from the indirect effects
563
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
aerosol types are considered (Figure 7.21). Although most model
estimates also include the direct and semi-direct effects, their
contribution to the TOA radiation is generally small compared
with the indirect effect, ranging from +0.1 to –0.5 W m
–2
due
to variations in the locations of black carbon with respect to
the cloud (Lohmann and Feichter, 2005). The simulated cloud
lifetime effect in a subset of models displayed in Figure 7.21
varies between –0.3 and –1.4 W m
–2
(Lohmann and Feichter,
2005), which highlights some of the differences among models.
The importance of the cloud albedo effect compared with the
cloud lifetime effect varies even when the models use the same
aerosol
fi
elds (Penner et al., 2006). Other differences among the
simulations include an empirical treatment of the relationship
between aerosol mass and cloud droplet number concentration
vs. a mechanistic relationship, the dependence of the indirect
aerosol effect on the assumed background aerosol or cloud droplet
number concentration, and the competition between natural and
anthropogenic aerosols as CCN (Ghan et al., 1998; O’Dowd
et al., 1999). Likewise, differences in the cloud microphysics
scheme, especially in the auto-conversion rate, cause different
cloud responses (e.g., A. Jones et al., 2001; Menon et al., 2002a,
2003; Penner et al., 2006).
All models agree that the total aerosol effect is larger over
the NH than over the SH (Figure 7.21). The values of the NH
total aerosol effect vary between –0.5 and –3.6 W m
–2
and
in the SH between slightly positive and –1.1 W m
–2
, with an
average SH to NH ratio of 0.3. Estimates of the ocean/land
partitioning of the total indirect effect vary from 0.03 to 1.8 with
an average value of 0.7. While the combined European Centre
for Medium Range Weather Forecasts/Max-Planck Institute for
Meteorology Atmospheric GCM (ECHAM4) plus Polarisation
and Directionality of the Earth’s Re
fl
ectance (POLDER)
satellite estimate suggests that the total aerosol effect should
be larger over oceans (Lohmann and Lesins, 2002), combined
estimates of the Laboratoire de Météorologie Dynamique
(LMD) and ECHAM4 GCMs with Moderate Resolution
Imaging Spectroradiometer (MODIS) satellite data reach the
opposite conclusion (Quaas et al., 2006). The average total
aerosol effect over the ocean of –1 W m
–2
agrees with estimates
of between –1 and –1.6 W m
–2
from the Advanced Very High
Resolution Radiometer (AVHRR)/POLDER (Sekiguchi et al.,
2003). Estimates from GCMs of the total aerosol effect are
generally larger than those from inverse models (Anderson et
al., 2003 and Chapter 9).
As compared with the estimates of the total aerosol effect
in Lohmann and Feichter (2005), some new estimates (Chen
and Penner, 2005; Rotstayn and Liu, 2005; Lohmann and Diehl,
2006) now also include the in
fl
uence of aerosols on the cloud
droplet size distribution (dispersion effect; Liu and Daum,
2002). The dispersion effect refers to a widening of the size
distribution in the polluted clouds that partly counteracts the
reduction in the effective cloud droplet radius in these clouds.
Thus, if the dispersion effect is taken into account, the indirect
cloud albedo aerosol effect is reduced by 12 to 42% (Peng and
Lohmann, 2003; Rotstayn and Liu, 2003; Chen and Penner,
2005). The global mean total indirect aerosol effect in the
simulation by Rotstayn and Liu (2005) has also been reduced
due to a smaller cloud lifetime effect resulting from a new
treatment of auto-conversion.
Global climate model estimates of the change in global mean
precipitation due to the total aerosol effects are summarised in
Figure 7.22. Consistent with the con
fl
icting results from detailed
cloud system studies, the change in global mean precipitation
varies between 0 and –0.13 mm day
–1
. These differences
are ampli
fi
ed over the SH, ranging from –0.06 mm day
–1
to
0.12 mm day
–1
. In general, the decreases in precipitation are
larger when the atmospheric GCMs are coupled to mixed-layer
ocean models (green bars), where the sea surface temperature
and, hence, evaporation are allowed to vary.
7.5.3
Effects of Aerosols and Clouds on Solar
Radiation at the Earth’s Surface
By increasing aerosol and cloud optical depth, anthropogenic
emissions of aerosols and their precursors contribute to a
reduction of solar radiation at the surface. As such, worsening
air quality contributes to regional aerosol effects. The partially
con
fl
icting observations on solar dimming/brightening are
discussed in detail in Section 3.4 and Box 3.2. This section
focuses on the possible contribution by aerosols. The decline
in solar radiation from 1961 to 1990 affects the partitioning
between direct and diffuse solar radiation: Liepert and Tegen
(2002) concluded that over Germany, both aerosol absorption
and scattering must have declined from 1975 to 1990 in order
to explain the simultaneously weakened aerosol forcing and
increased direct/diffuse solar radiation ratio. The direct/diffuse
solar radiation ratio over the USA also increased from 1975 to
1990, likely due to increases in absorbing aerosols. Increasing
aerosol optical depth associated with scattering aerosols
alone in otherwise clear skies produces a larger fraction of
diffuse radiation at the surface, which results in larger carbon
assimilation into vegetation (and therefore greater transpiration)
without a substantial reduction in the total surface solar radiation
(Niyogi et al., 2004; Section 7.2.6.2).
For the tropical Indian Ocean, Ramanathan et al. (2001)
estimate an indirect aerosol effect of –5 W m
–2
at TOA and
–6 W m
–2
at the surface. While the direct effect is negligible at TOA,
its surface forcing amounts to –14 W m
–2
as a consequence of large
atmospheric absorption in this region. In South Asia, absorbing
aerosols may have masked up to 50% of the surface warming
due to the global increase in greenhouse gases (Ramanathan et
al., 2005). Global climate model estimates of the mean decrease
in surface shortwave radiation in response to all aerosol effects
vary between –1.3 and –3.3 W m
–2
(Figure 7.23). It is larger
than the TOA radiation
fl
ux change because some aerosols like
black carbon absorb solar radiation within the atmosphere (see
also Jacobson, 2001; Lohmann and Feichter, 2001; Ramanathan
et al., 2001; Liepert et al., 2004). As for the TOA net radiation,
the decrease is largest over land, with values approaching
–9 W m
–2
. Consistent with the above-mentioned regional studies,
most models predict larger decreases over land than over the
oceans.
564
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
Figure 7.22.
Global mean change in precipitation due to the total anthropogenic aerosol effect (direct, semi-direct and indirect cloud albedo and lifetime effects) from pre-
industrial times to the present day and its contribution over the NH and SH, over oceans and over land. Red bars refer to anthropogenic sulphate (Easter et al., 2004; Ming et
al., 2005
+
), blue bars to anthropogenic sulphate and organic carbon (Quaas et al., 2004; Rotstayn and Liu, 2005
+
), cyan bars to anthropogenic sulphate, and black and organic
carbon (Menon and Del Genio, 2005; Takemura et al., 2005; Johns et al., 2006; Storelvmo et al., 2006), dark purple bars to anthropogenic sulphate and black and organic
carbon effects on water and ice clouds (Jacobson, 2006; Lohmann and Diehl, 2006), teal bars refer to a combination of GCM and satellite results (LMDZ/ECHAM plus MODIS,
Quaas et al., 2006), green bars refer to results from coupled atmosphere/mixed-layer ocean (MLO) experiments (Feichter et al., 2004: sulphate and black and organic carbon;
Kristjansson et al., 2005: sulphate and black carbon; Rotstayn and Lohmann, 2002
+
: sulphate only) and olive bars to the mean from all simulations. Vertical black lines refer to
±1 standard deviation.
+
refers to estimates solely from the indirect effects
Transient simulations (Roeckner et al., 1999) and coupled
GCM-mixed-layer ocean equilibrium simulations (Feichter et
al., 2004; Liepert et al., 2004) suggest that the decrease in solar
radiation at the surface resulting from increases in optical depth
due to the direct and indirect anthropogenic aerosol effects is
more important for controlling the surface energy budget than
the greenhouse-gas induced increase in surface temperature.
There is a slight increase in downwelling longwave radiation
due to aerosols, which in the global mean is small compared
to the decrease in shortwave radiation at the surface. The other
components of the surface energy budget (thermal radiative
fl
ux, sensible and latent heat
fl
uxes) decrease in response to the
reduced input of solar radiation. As global mean evaporation
must equal precipitation, a reduction in the latent heat
fl
ux in the
model leads to a reduction in precipitation (Liepert et al., 2004).
This is in contrast to the observed precipitation evolution in the
last century (see Section 3.3) and points to an overestimation
of aerosol in
fl
uences on precipitation. The simulated decrease
in global mean precipitation from pre-industrial times to the
present may reverse into an increase of about 1% in 2031 to 2050
as compared to 1981 to 2000, because the increased warming
due to black carbon and greenhouse gases then dominates over
the sulphate cooling (Roeckner et al., 2006).
7.5.4
Effects of Aerosols on Circulation Patterns
7.5.4.1
Effects on Stability
Changes in the atmospheric lapse rate modify the longwave
emission and affect the water vapour feedback (Hu, 1996) and
the formation of clouds (see, e.g., Section 8.6). Observations and
model studies show that an increase in the lapse rate produces
an ampli
fi
cation of the water vapour feedback (Sinha, 1995).
As aerosols cool the Earth’s surface and warm the aerosol layer,
the lapse rate will decrease globally and suppress the water
vapour feedback (e.g., Feichter et al., 2004). The local change
565
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Figure 7.23.
Global mean change in net solar radiation at the surface due to the total anthropogenic aerosol effect (direct, semi-direct and indirect cloud albedo and lifetime
effects) from pre-industrial times to the present day and its contribution over the NH and SH, over oceans and over land and the ratio over oceans/land. Red bars refer to
anthropogenic sulphate (Easter et al., 2004; Ming et al., 2005
+
), blue bars to anthropogenic sulphate and organic carbon (Quaas et al., 2004; Rotstayn and Liu, 2005
+
), cyan
bars to anthropogenic sulphate and black and organic carbon (Menon and Del Genio, 2005; Takemura et al., 2005; Johns et al., 2006; Storelvmo et al., 2006), dark purple bars
to anthropogenic sulphate and black and organic carbon effects on water and ice clouds (Jacobson, 2006; Lohmann and Diehl, 2006), teal bars refer to a combination of GCM
and satellite results (LMDZ/ECHAM plus MODIS, Quaas et al., 2006), green bars refer to results from coupled atmosphere/mixed-layer ocean (MLO) experiments (Feichter et al.,
2004: sulphate and black and organic carbon; Kristjansson et al., 2005: sulphate and black carbon; Rotstayn and Lohmann, 2002
+
: sulphate only) and olive bars to the mean
from all simulations. Vertical black lines refer to ±1 standard deviation.
+
refers to estimates solely from the indirect effects
in atmospheric stability strongly depends on the altitude of the
black carbon heating (Penner et al., 2003).
Absorption of solar radiation by aerosols can change the
cloud amount (semi-direct effect; Grassl, 1975; Hansen et
al.,
1997; Ackerman et al.,
2000;
Ramanathan et al.,
2001;
Jacobson, 2006; Figure 7.20). The semi-direct effect has been
simulated with GCMs and high-resolution cloud-resolving
models, since it is implicitly accounted for whenever absorbing
aerosols coupled to the radiation scheme are included (Hansen
et al.,
1997; Lohmann and Feichter,
2001; Jacobson,
2002;
Menon et al.,
2002b; Penner et al.,
2003; Cook and Highwood,
2004; Hansen et al.,
2005). Aerosol heating within cloud layers
reduces cloud fractions, whereas aerosol heating above the
cloud layer tends to increase cloud fractions. When diagnosed
within a GCM framework, the semi-direct effect can also
include cloud changes due to circulation effects and/or surface
albedo effects. Moreover, the semi-direct effect is not exclusive
to absorbing aerosol, as potentially any radiative heating of
the mid-troposphere can produce a similar response in a GCM
(Hansen et al.,
2005; see
also Section 2.8). Cloud-resolving
models of cumulus and stratocumulus case studies also diagnose
semi-direct effects indicating a similar relationship between the
height of the aerosol layer relative to the cloud and the sign of
the semi-direct effect (Ackerman et al.,
2000; Ramanathan et al.,
2001; Johnson et al.,
2004; Johnson,
2005). Using a large eddy
simulation, Feingold et al. (2005) show that the reduction in net
surface radiation and in surface latent and sensible heat
fl
uxes
is the most simple explanation of the reduction in cloudiness
associated with absorbing aerosols.
7.5.4.2
Effects on the Large-Scale Circulation
Several studies have considered the response of a GCM
with a mixed-layer ocean to indirect aerosol effects (Rotstayn
et al., 2000; K. Williams et al., 2001; Rotstayn and Lohmann,
2002) or to a combination of direct and indirect aerosol effects
566
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
(Feichter et al., 2004; Kristjansson et al., 2005; Takemura et al.,
2005). All of these, and recent transient simulations (Held et
al., 2005; Paeth and Feichter, 2006), found a substantial cooling
that was strongest in the NH, with a consequent southward
shift of the Inter-Tropical Convergence Zone (ITCZ) and the
associated tropical rainfall belt. Rotstayn and Lohmann (2002)
even suggest that aerosol effects might have contributed to the
Sahelian droughts of the 1970s and 1980s (see Sections 9.5 and
11.2). If in turn the NH is warmed, for instance due to the direct
forcing by black carbon aerosols, the ITCZ is found to shift
northward (Chung and Seinfeld, 2005).
Menon et al. (2002b) and Wang (2004) found that
circulation changes could be caused by aerosols in southeast
China. In India and China, where absorbing aerosols have been
added, increased rising motions are seen as well as increased
subsidence to the south and north (Menon et al., 2002b).
However, Ramanathan et al. (2005) found that convection
was suppressed due to increased stability resulting from black
carbon heating. Drier conditions resulting from suppressed
rainfall can induce more dust and smoke due to the burning of
drier vegetation (Ramanathan et al., 2001), thus affecting both
regional and global hydrological cycles (Wang, 2004). Heating
of a lofted dust layer could increase the occurrence of deep
convection (Stephens et al., 2004). It can also strengthen the
Asian summer monsoon circulation and cause a local increase
in precipitation, despite the global reduction of evaporation that
compensates aerosol radiative heating at the surface (Miller et
al., 2004b). The dust-induced thermal contrast changes between
the Eurasian continent and the surrounding oceans are found
to trigger or modulate a rapidly varying or unstable Asian
winter monsoon circulation, with a feedback to reduce the dust
emission from its sources (Zhang et al., 2002).
In summary, an increase in atmospheric aerosol load
decreases air quality and reduces the amount of solar radiation
reaching the surface. This negative radiative forcing competes
with the greenhouse gas warming for determining the change in
evaporation and precipitation. At present, no transient climate
simulation accounts for all aerosol-cloud interactions, so that
the net aerosol effect on clouds deduced from models is not
conclusive.
7.6 Concluding
Remarks
Biogeochemical cycles interact closely with the climate
system over a variety of temporal and spatial scales. On
geological time scales, this interaction is illustrated by the
Vostok ice core record, which provides dramatic evidence of
the coupling between the carbon cycle and the climate system.
The dynamics of the Earth system inferred from this record
result from a combination of external forcing (in this case long-
term periodic changes in the orbital parameters of the Earth
and hence solar forcing) and an array of feedback mechanisms
within the Earth environment (see Chapter 6). On shorter time
scales, a range of forcings originating from human activities
(conversion and fragmentation of natural ecosystems, emissions
of greenhouse gases, nitrogen
fi
xation, degradation of air quality,
stratospheric ozone depletion) is expected to produce planet-
wide effects and perturb numerous feedback mechanisms that
characterise the dynamics of the Earth system.
A number of feedbacks that amplify or attenuate the climate
response to radiative forcing have been identi
fi
ed. In addition to
the well-known positive water vapour and ice-albedo feedbacks,
a feedback between the carbon cycle and the climate system
could produce substantial effects on climate. The reduction in
surface carbon uptake expected in future climate should produce
an additional increase in the atmospheric CO
2
concentration and
therefore enhance climate forcing. Large differences between
models, however, make the quantitative estimate of this
feedback uncertain. Other feedbacks (involving, for example,
atmospheric chemical and aerosol processes) are even less
well understood. Their magnitude and even their sign remain
uncertain. Potentially important aerosol-cloud interactions such
as changes in cloud lifetime and aerosol effects on ice clouds
can in
fl
uence the hydrologic cycle and the radiative budget;
however, the scienti
fi
c understanding of these processes is low.
The response of the climate system to anthropogenic forcing
is expected to be more complex than simple cause and effect
relationships would suggest; rather, it could exhibit chaotic
behaviour with cascades of effects across the different scales
and with the potential for abrupt and perhaps irreversible
transitions.
This chapter has assessed how processes related to
vegetation dynamics, carbon exchanges, gas-phase chemistry
and aerosol microphysics could affect the climate system.
These processes, however, cannot be considered in isolation
because of the potential interactions that exist between them.
Air quality and climate change, for example, are intimately
coupled (Dentener et al., 2006). Brasseur and Roeckner (2005)
estimate that the hypothetical removal from the atmosphere of
the entire burden of anthropogenic sulphate aerosol particles
(in an effort to improve air quality) would produce a rather
immediate increase of about 0.8°C in the globally averaged
temperature, with geographical patterns that bear a resemblance
to the temperature changes found in greenhouse gas scenario
experiments (Figure 7.24). Thus, environmental strategies
567
Chapter 7
Couplings Between Changes in the Climate System and Biogeochemistry
Figure 7.24.
Effect of removing the entire burden of sulphate aerosols in the year
2000 on (a) the annual mean clear sky TOA shortwave radiation (W m
–2
) calculated
by Brasseur and Roeckner (2005) for the time period 2071 to 2100 and (b) on the
annual mean surface air temperature (°C) calculated for the same time period. (c)
temporal evolution of global and annual mean surface air temperature anomalies (°C)
with respect to the mean 1961 to 1990 values. The evolution prior to the year 2000
is driven by observed atmospheric concentrations of greenhouse gases and aerosols
as adopted by IPCC (see Chapter 10). After 2000, the concentration of greenhouse
gases remains constant while the aerosol burden is unchanged (blue line) or set to
zero (red line). The black curve shows observations (A. Jones et al., 2001; Jones et
al., 2006).
aimed at maintaining ‘global warming’ below a prescribed
threshold must therefore account not only for CO
2
emissions
but also for measures implemented to improve air quality. To
cope with the complexity of Earth system processes and their
interactions, and particularly to evaluate sophisticated models
of the Earth system, observations and long-term monitoring
of climate and biogeochemical quantities will be essential.
Climate models will have to reproduce accurately the important
processes and feedback mechanisms discussed in this chapter.
568
Couplings Between Changes in the Climate System and Biogeochemistry
Chapter 7
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