climate change paradigms jan 2010m - world...
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Responding to Climate Change: the need for a paradigm shift
Diane L. Douglas, Ph.D., RPA
Abstract Global warming is one of the most important and dangerous issues facing man today. Many scientists and politicians have focused on anthropogenic causes of this change and the need to reduce CO2 emissions to limit or slow the process. Major climate changes, however, have occurred throughout earth’s history. The shifting of continental plates, rise of mountains, and cyclical changes in earth’s orbit around the sun are primary forcing mechanisms driving climate change. The complex coupling between the atmosphere, ocean, clouds, ice sheets, volcanoes, earthquakes, and the exchange of carbon within living organisms also affect climate. Over the past two million years, earth’s climate has been punctuated by glacial and interglacial periods—periods when earth’s temperature ranged from 8oC cooler to 4oC warmer than present. Hominids adapted their settlements and subsistence practices to these changes. Modern humans evolved around 40,000 years ago, during the last ice age, and at the end of the last ice age migrated to new lands and new continents. People developed new technologies and adaptive strategies in response to sea level rise and a more productive environment. Today we face climate change of a similar magnitude to the last interglacial. This paper shows how natural forcing mechanisms may drive earth into an interglacial as warm as the last interglacial, regardless of reductions in greenhouse gas emissions. Sea level may rise 4.6 – 6 m (15 – 20 ft), and in some regions storms will increase in frequency and strength, and in others deserts will expand. In order to plan appropriate responses climate change we must first obtain a comprehensive understanding of natural forcing mechanisms and how anthropogenic activities accentuate these mechanisms. At present there are two schools of thought: 1) anthropogenic burning of fossil fuels and land use practices are driving global warming; and 2) earth is experiencing a natural climate cycle, similar to cycles that have occurred in the past. The first argument is dismissed by some as being too simplistic—earth’s climate is driven by complex dynamics and recent warming can not be entirely explained by anthropogenic emissions of CO2 and other greenhouse gases. The second argument is dismissed by others because the rate of global warming observed in the past fifty years exceeds warming documented in historic records, or reconstructed further back in history using proxy data. This paper discusses the current state of scientific knowledge of global warming, and argues that the current state of knowledge is inadequate for developing reliable estimates of future climate change. The technical reports prepared by the intergovernmental panel for climate change (IPCC) are reviewed, gaps in knowledge identified by these authors are discussed, and recommendations for future research are proffered.
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Table of Contents Abstract ........................................................................................................................................... 1 Introduction..................................................................................................................................... 3
Organization of this Paper .......................................................................................................... 5 The Global Warming Debate .......................................................................................................... 6 Earth’s Energy Balance................................................................................................................... 9
Variation in Earth’s Energy Balance ........................................................................................ 10 Photosynthesis....................................................................................................................... 10 CO2 Pressure in the Ocean versus Atmosphere .................................................................... 11 Albedo................................................................................................................................... 11 Tectonics and Volcanism...................................................................................................... 12 Atmospheric Circulation....................................................................................................... 15 Intertropical Convergence Zone (ITCZ)............................................................................... 16 Oceanic Circulation .............................................................................................................. 17 Changes in Atmospheric and Oceanic Circulation ............................................................... 18 Temporal Variations in Atmospheric and Oceanic Circulation............................................20 Celestial Mechanics .............................................................................................................. 20
Climate Models............................................................................................................................. 24 The IPCC Climate Models........................................................................................................ 26 Climate Models of the Past for Predicting the Future............................................................... 27
IPCC and Ocean Acidity....................................................................................................... 29 Verifying Climate Models ........................................................................................................ 30
Reconstructing Past Environments to Predict the Future ............................................................. 32 Proxy Data ................................................................................................................................ 32
Tree Rings as Proxy Data ..................................................................................................... 35 Pollen as Proxy Data............................................................................................................. 36 Macrobotanical Materials as Proxy Data.............................................................................. 36 Isotopes as Proxy Data.......................................................................................................... 38
Proxy Data Limitations............................................................................................................. 41 Limitations of Tree-Rings and Macrobotanical Data ........................................................... 42 Limitations of Isotopes: Ice Cores and Foraminifera........................................................... 42
Archaeology, History and Climate Change .................................................................................. 46 Economics of Greenhouse Gas Policies ....................................................................................... 47 Discussion..................................................................................................................................... 48
Punctuated Equilibrium and the Threshold Effect.................................................................... 49 Research Suggestions.................................................................................................................... 51
Paleoenvironmental Reconstructions........................................................................................ 51 Modeling................................................................................................................................... 52
Conclusions................................................................................................................................... 52 References..................................................................................................................................... 54 Appendix 1.................................................................................................................................... 66 Climate Models and Their Parameters.......................................................................................... 66
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Introduction
Global warming is one of the most important and dangerous issues facing man today. Many
scientists and politicians have focused on anthropogenic causes of this change and the need to
reduce CO2 emissions to limit or slow the process. For several years, many scientists have
argued that anthropogenic greenhouse gas (GHG) emissions and land use practices are the
primary forcing mechanism driving current global warming. The idea that people are the primary
cause of global warming as observed in worldwide temperature records is based on reports from
the Intergovernmental Panel of Climate Change (ICPP). The IPCC was established in 1988 by
the United Nations Environment Programme (UNEP) and the World Meteorological
Organization (WMO), both of which are a part of the United Nations (IPCC 2008). This
organization was formed to review and summarize climate studies that analyze the affects of
anthropogenic GHG emissions, including carbon dioxide (CO2), methane (CH4), nitrous oxide
(N2O) and various chlorofluorocarbons (CFCs), and human land use on climate change. Human
land use is an important consideration in climate change studies because deforestation removes
trees and plants that convert CO2 to oxygen (O2) through photosynthesis.
In order to understand how different trace gases affect global warming, the heat potential of CO2,
CH4, N2O and CFC and other miscellaneous gases have been analyzed (United States
Department of Energy (DOE) 2000). The analysts determined that CO2 has the highest potential
for retaining heat, and that relative to other trace gases in the atmosphere it contributes 72.34% to
global warming. The IPCC reports indicate that anthropogenic emissions of CO2 is increasing
the %age of CO2 in the atmosphere, which is causing the atmosphere to warm at a faster rate
than would occur under natural conditions (Forster et al. 2007; Jansen et al. 2007; Randall et al.
2007). Because CO2 retains considerably more heat than CH4, N2O or CFCs, the IPCC has
warned policymakers that if anthropogenic emissions of CO2 are not reduced and maintained at
levels pre-dating 1990, the earth will warm by up to 6.1oC between 2060 and 2090 (Barker et al.
2007:39). Warming of this magnitude replicates the degree of warming that scientists have
determined occurred during the last interglacial period, between 125,000 and 115,000 years ago.
Sea level during this period was approximately 5m (16 ft) higher than present—a level that will
result in devastating flooding of major coastal cities such as Venice, Italy, New York, New York,
and St. Petersburg, Florida. In addition to these heavily populated areas, many coastal natural
world heritage sites that contribute to earth’s rich biodiversity and beauty will be inundated.
World heritage cultural sites located along coastlines subjected to erosion and intense storms will
also be destroyed and lost to future generations.
In addition to direct impacts on coastal cities, estuaries, beaches and cultural sites, warming of
this magnitude has the potential to affect changes in atmospheric and oceanic circulation,
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resulting in more intense storms in some regions and drought in others. Changes in atmospheric
and oceanic circulation will also affect the distribution of arable lands and the distribution of
shellfish, fish, and other marine organisms that people rely upon for food. The IPCC panel
predicts devastating effects to the world economy as a result of stresses to global food and
potable water supplies, and social and political stresses associated with the need to relocate
millions of people from coastal communities and low-lying islands.
The economic and social implications of global warming have spurred policymakers to request
guidance from economists and scientists on how to slow, and ultimately stop global warming.
To return CO2 in the atmosphere to pre-1990 levels, governments of developed nations have
invested billions of dollars to identify the technological means to reduce global greenhouse gas
emissions. Nearly all of the member nations of the United Nations have ratified the Kyoto
Protocol, a measure established by the United Nations Framework Convention on Climate
Change (UNFCCC) which legally binds ratifying countries to control their GHG emissions
(UNFCCC 2008). To achieve this goal, however, several billion more dollars will need to be
spent to develop new sources of energy and modify industry, vehicles, and homes to be more
energy efficient. In the United States alone it is estimated that the cost to ratify the Kyoto
Protocol would be approximately 400 hundred billion dollars and result in a loss of roughly 4.9
million jobs (Daynes and Sussman 2006). Further, consultants to UNEP report that in response to
climate change over $ 210 billion dollars will be invested annually by 2030 to mitigate and
develop a sustainable energy supply infrastructure (UNEP 2008:9). Given the financial cost of
responding to global warming, communities worldwide can hope that the Kyoto Protocol and
other measures being implemented to reduce anthropogenic GHG emissions and minimize
deforestation will have a significant impact on slowing and/or stopping global warming.
The current worldwide recession makes it clear that the world’s financial resources are limited,
and we must be efficient and effective in our actions to combat and respond to global warming.
Some scientists argue, however, that we are not adequately considering natural forcing
mechanisms that may be the underlying cause of much of the global warming observed in recent
decades. The scientific studies reviewed and reported upon by the IPCC Fourth Working Group
(Barker et al. 2007; IPCC 2007a and IPCC 2007b; Jansen et al. 2007; Forster et al. 2007; Randall
et al. 2007), document multiple areas where the research reviewed does not conclude with
certainty that anthropogenic GHG emissions and land use practices are the primary forcing
mechanism causing recent global warming. These scientists note that additional research must be
performed to understand the complex interaction of anthropogenic behavior and natural forcing
mechanisms (Jansen et al. 2007; Randall et al. 2007; Meehl et al. 2007). For example, the
climate models used to simulate future climate could not fully integrate natural climate forcing
mechanisms because of time and cost constraints, as well as limited knowledge of some physical
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processes (Jansen et al. 2007; Randall et al. 2007). The Fourth Working Group technical reports
were summarized by the IPCC (e.g., Barker et al. 2007; IPCC 2007a and 2007b). Although these
summaries recognize uncertainties in the technical reports, they state that the scientific evidence
overwhelmingly indicates people are having a significant impact on global warming; these
reports are being used to guide the UNFCCC on how global climate change should be addressed
(Barker et al. 2007; IPCC 2007a and 2007b).
This paper summarizes the current state of knowledge of climate change based on the IPCC
technical reports (Forster et al. 2007; Jansen et al. 2007; Randall et al. 2007), as well as
independent studies (e.g. Hirst 1999; Giorgi and Mearns 2001; Freidenreich and Ramaswamy
2005; Gregory et al. 2005; Hall et al. 2005; Berger et al. 2006). Gaps in knowledge regarding
global climate change identified by these scientists are summarized. Natural forcing mechanisms
that may be contributing to the rapid climate change observed over the past 50 years are
highlighted (e.g. Trogler et al. 1997; Patterson 2005), and additional research that might fill the
data gaps identified by the IPCC are discussed. In addition to the IPCC technical reports, over
150 scientific papers were reviewed by the author of this paper in an effort to bridge the gap
between what is known about anthropogenic forcing of global warming and natural forcing of
global warming. The author’s intent is to highlight areas where additional research is needed to
better understand the natural mechanisms that are accentuating anthropogenic affects of climate
change. This research was performed to inform policymakers that the current approaches to
combating and responding to global warming may not be sufficient to prepare world
communities to climate change that may be imminent. The author’s objective is to provide
policymakers with information that can be used to direct use of the world’s limited financial
resources more efficiently and effectively than is currently planned. No money was accepted
from any parties for the research or writing of this report—additionally the report was prepared
by the author on time off from work and does not reflect the views of her employer.
Organization of this Paper
This paper places anthropogenic causes of global within the context of natural forcing
mechanisms that have driven climate change over millions of years. The first section of the
paper summarizes the history of socio-political and scientific concerns regarding the impacts of
anthropogenic aerosol pollutants on human health and the environment. The next section
discusses the balance between incoming solar radiation from the sun and outgoing long wave
radiation emitted from earth, and highlights how earth’s atmosphere functions. The following
section summarizes the physical processes that affect climate variability on different temporal
and spatial scales. The next section explains how information on earth’s physical dynamics is
used to develop climate models that reconstruct past climates and simulate future climate change.
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Methods used to verify the accuracy and reliability of these models is then reviewed. The next
section discusses climate models used by the IPCC Fourth Working Group to simulate climate
change under different socio-economic and technological scenarios (Randall et al. 2007).
Inadequacies of these models to predict future climate change is also summarized (Randall et al.
2007). The following section summarizes the types of environmental data (proxy data) used to
verify models of past climates (Jansen et al. 2007) and the limitations of these data for
reconstructing climate conditions at different temporal and spatial scales (Schwander and
Stauffer 1984; Mix and Ruddiman 1984; Stauffer et al. 1985; Mix 1987; Barnola et al. 1991;
Petit et al. 1999; Jansen et al. 2007; Fontanier et al 2008). Following this the economic and social
implications of global warming induced by anthropogenic and natural forcing mechanisms are
discussed (Forster et al. 2007; IPCC 2007; Meehl et al. 2007). Finally, research that could
provide greater understanding of the magnitude of current global warming caused by natural
forcing mechanisms is proposed.
The Global Warming Debate Scientists first became concerned that anthropogenic activities were having an adverse effect on
the atmosphere in the 1950s when they began identifying adverse affects of anthropogenic
aerosols (CO2, CH4, N2O and CFCs) on human health, agricultural productivity and livestock. In
response to this discovery, the United States Congress passed the Air Pollution Control Act
(1955, public law 84-159) and over the next eight years implemented two amendments,
encouraging additional research on the impacts of aerosols on human health and the
environment. In 1963 the United States Congress passed the Clean Air Act (public law 88-206)
and granted 95 million dollars to conduct additional research and develop programs to control
aerosol emissions. Over the next 27 years, scientists identified increasing adverse effects of air
pollutants to human health and the environment (American Meteorological Society 2008). Prior
to publicity regarding the effects of anthropogenic GHG emissions on global warming, the most
widely publicized discovery was the affect of CFCs on the ozone layer. This layer of natural
atmospheric gas (O3) is located in the stratosphere and absorbs approximately 95% of the sun’s
ultraviolet light, which can cause an increase in skin cancer, as well as damage livestock, crops,
plankton and algae. When policymakers became aware of the imminent threat on human life, the
U.S. Congress amended the Clean Air Act (1990, public law 101-549) and mandated adoption of
best available control technologies to reduce CFC emissions.
Around this same time, the UNEP and WMO formed the IPCC to study the extent to which
human land use practices and anthropogenic GHG emissions are causing global warming (IPCC
2009). Since 1988, the IPCC has performed an extensive review of scientific studies on climate
change and prepared exhaustive reports detailing the results of these reviews. The IPCC is
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organized into three working groups, one which summarizes the physical sciences of climate
change, another which summarizes the vulnerability of human and natural systems to climate
change, and a third which evaluates mitigation measures to reduce or control GHG emissions
(IPCC 2009). It is important to note that these scientists do not perform independent research,
but rather review the results of studies performed by other scientists.
The first IPCC technical report series was released in 1990, and its findings were key in
establishing the Intergovernmental Negotiating Committee (INC) for the United Nations
Framework Convention on Climate Change (UNFCCC). The IPCC’s second report was released
in 1995, and their statement that, “[t]he balance of evidence suggests a discernible human
influence on global climate,” contributed significantly to the formation and adoption of the
Kyoto Protocol (IPCC 2009). The third and fourth assessment reports, released in 2001 and
2007 respectively, contributed even more to the perception that human land use (deforestation,
desertification, draining of wetlands, and expansion of cities) and anthropogenic GHG emissions
from industry and vehicles are major forcing mechanisms in global warming.
Based on the early findings of the IPCC, the United Nations gave the UNFCCC the task of
promoting the adoption of best available control technologies to reduce GHG emissions. Within
a few years of being formed, 192 of the member nations of the United Nations ratified the
UNFCCC and pledged to limit or reduce their GHG emissions. The release of the first IPCC
reports made scientists and policymakers aware of the amounts of anthropogenic GHG emissions
being emitted into the atmosphere relative to natural volumes of GHG emissions and the
UNFCCC adopted more extreme measures to reduce anthropogenic GHG emissions. In 1997 the
UNFCCC adopted the Kyoto Protocol which legally binds ratifying countries to control their
GHG emissions (UNFCCC 2008).
Concurrent with the IPCC investigations of human-induced global warming, other climate
scientists have argued that anthropogenic GHG emissions contribute less than 1% to global
warming, and that natural and anthropogenic CO2 combined contribute only 3.62% to
greenhouse warming (Trogler et al. 1997; Patterson 2005). Chemical analyses of the heat
retention characteristics of atmospheric trace gases and water vapor have determined that the
heat retention characteristics of water vapor are much higher than that of CO2 (see the United
States Department of Energy [DOE] 2000); atmospheric physicists note that water vapor retains
95% of the heat in the atmosphere (Trogler et al. 1997). Based on these findings, and the fact that
CO2 comprises less than 0.04% of the atmosphere and water vapor comprises 1% several
scientists have argued that changes in the amount of water vapor in the atmosphere must be
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driving the rate and magnitude of global warming that has occurred since AD 1850 (see for
example Trogler et al. 1997; Essenhigh 2001; Jaworowski 2004; Patterson 2005).
However, the arguments presented by these scientists are often dismissed without serious
consideration, their critics claiming that the research performed by these scientists must have
been financed by big industry, biasing their results (Gore 2006; Michaels 2008, Reinhard 2008).
However, the much of the data reported upon by these scientists are derived from United States
federal agencies, and these data are available to the public (and scientists) for review,
consideration and analysis. These agencies include the: National Oceanic and Atmospheric
Administration (NOAA); National Center for Atmospheric Research (NCAR); Carbon Dioxide
Information Analysis Center of the United States DOE; and National Aeronautics and Space
Administration (NASA). Public links for these organizations and their data are presented in the
references section of this paper; these data were used by the author to develop several of the
graphs and charts presented in this paper.
Dismissing the arguments of climate scientists who state earth’s natural forcing mechanisms are
the primary cause of global warming out-of-hand does not do justice to the scientific process.
Perhaps more critically, it suggests policymakers are not giving full consideration to the natural
forcing mechanisms driving global warming. The statements made by these scientists should be
evaluated with the rigor applied to the scientific studies reviewed and reported upon by the
IPCC. The IPCC’s “role is to assess on a comprehensive, objective, open and transparent basis
the latest scientific, technical and socio-economic literature produced worldwide relevant to the
understanding of the risk of human-induced climate change” (IPCC 2009, emphasis added).
Relative to this mandate, the IPCC reports are extremely comprehensive (Forester et al. 2007;
Jansen et al. 2007; Randall et al. 2007; Meehl et al. 2007).
However, given that the policies adopted by the world’s leading nations will affect all life on
earth as well as the global economy for generations to come, perhaps natural forcing mechanisms
should be given full consideration in the analysis of climate change: present and future. These
natural mechanisms combined with anthropogenic effects may result in even more extreme
conditions than the UNFCCC and its member nations are currently considering. Earth’s physical
processes and the dynamics of earth’s energy balance that drive the CO2 cycle and climate
change are very complex, as are the climate models that are used to simulate climate change.
Below, the physical processes that drive earth’s energy balance are reviewed to provide a
framework for understanding natural forcing mechanisms that drive climate change. This
information provides a context for understanding the additional research that the IPCC Fourth
Working Group identifies as necessary for developing a more comprehensive understanding of
climate change.
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Earth’s Energy Balance
Life on earth would not be possible without the energy received from the sun and the life-giving
air of our atmosphere. Earth’s atmosphere is composed of nitrogen (78.8%), oxygen (20.95%),
argon (0.93%), carbon dioxide (0.038%), various other trace gases and water vapor (1%). The
molecules associated with these gases have mass. Correspondingly, because of the effect of
gravity air is denser closer to the earth (such as at sea level) than it is higher in the atmosphere
(such as on top of Mount Everest). Understanding atmospheric pressure is important for
understanding climate change on seasonal to millennial time scales, because it affects how warm
air is distributed from the equator to the poles, as well as how warm and cold air is distributed
across continents. In climatology, air density is measured by atmospheric pressure and at sea
level mean atmospheric pressure is about 101300 pascals (1013 millibars: mbar). On top of
Mount Everest, roughly 8.9 kilometers (5.5 miles) above sea level, mean atmospheric pressure is
about 34000 pascals (340 mbar) (West 1999). Atmospheric pressure also varies temporally and
spatially across the globe in response to variations in incoming solar radiation and oceanic
circulation. These changes in atmospheric pressure cause changes in regional weather, including
everything from droughts, thunderstorms and tornadoes to hurricanes and monsoon rains.
The energy received from the sun as short wave radiation (insolation) is in delicate balance with
the energy emitted by earth as outgoing long wave radiation (Figure 1). The average amount of
energy received at the top of the atmosphere from the sun is approximately 1,366 watts per
square meter (W/m2), with the highest levels of radiation received at the equator. A marked
increase or decrease in insolation effects earth’s climate, and is the primary reason earth
experiences ice ages (glacial periods) and interglacial periods, such as today. Approximately 19
% of the sun’s shortwave radiation is absorbed by the earth’s atmosphere, and 51% is absorbed
by the land and water bodies (Pidwirny 2006a and 2006b); the remaining short wave radiation
(30%) is reflected back to space by particles in the atmosphere, clouds, and earth’s albedo.
Figure 1. Earth’s Energy Balance.
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For earth’s heat budget to remain in balance, the amount of incoming solar radiation absorbed by
the atmosphere and earth (70%) must be balanced by the same amount of outgoing longwave
radiation (70%). Radiation emitted by the earth is called longwave radiation because it is cooler
than the sun and emits longer wavelengths of energy. Approximately 70% of the longwave
radiation emitted by earth passes through the atmosphere and escapes to space. The remaining
30% is trapped by water vapor and aerosols (trace gases) in the atmosphere and warms the
earth—this is referred to as the greenhouse effect. The greenhouse effect makes life on earth
possible, but changes in the amount of aerosols and/or water vapor in the atmosphere can have a
marked effect on climate. Higher levels of trace gases (greenhouse gases) trap more longwave
radiation and effectively heat earth’s surface; a reduction in the levels of greenhouse gases
allows more long-wave radiation to escape, effectively cooling earth’s surface.
Variation in Earth’s Energy Balance
Variation in earth’s energy balance occurs over long and short time scales and in response to
multiple variables including changes in: 1) the amount of incoming solar radiation 2) earth’s CO2
cycle – photosynthesis and diffusion into the ocean, 3) albedo, 4) tectonic and volcanic activity,
5) atmospheric and oceanic circulation and 6) celestial mechanics. The contribution of each of
these systems to earth’s energy balance is discussed in greater detail below.
Photosynthesis
Energy from the sun drives photosynthesis in all land plants, algae and some types of
photosynthetic bacteria (Whitmarsh and Govinjee 1999). Photosynthesis converts CO2 from the
air and water (H2O) into O2 and carbohydrates (C6H12O6); O2 is utilized by all oxygen
consuming organisms on earth (Whitmarsh and Govinjee 1999:11). Deforestation and land
clearing therefore result in less CO2 being absorbed by plants, throwing off the natural balance of
earth’s CO2 cycle.
Whitmarsh and Govinjee (1999), note that absorption of CO2 by planktonic foraminifera in the
upper layers of the oceans removes approximately 2 x 1015 grams of carbon per year from the
atmosphere. The process is initiated by plankton photosynthesizing CO2 into organic carbon
(Whitmarsh and Govinjee 1999), as well as CO2 and H2O reacting to form HCO3 (carbonate
ions) which is absorbed by marine organisms to form shells of calcium carbonate (CaCO3). As
these organisms die, they sink to the bottom of the ocean where they settle into the sediment
(Whitmarsh and Govinjee 1999).
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The ocean contains approximately 19 and 50 times more CO2 than the terrestrial biosphere,
atmosphere, respectively (Sabine 2008). In Polar waters, CO2 absorption is highest during the
summer when the Arctic regions are blanketed in flora; absorption decreases during winter
because of ice cover (Tans et al. 1990; Primack 2004).
CO2 Pressure in the Ocean versus Atmosphere
In addition to CO2 being absorbed by planktonic foraminifera, CO2 is absorbed by the upper
layers of the ocean when the CO2 gas pressure (pCO2) in the atmosphere is higher than the pCO2
in the ocean’s upper layers (Sabine 2008). In high latitudes, CO2 flows from the atmosphere into
the ocean and in the tropics CO2 is released from the ocean to the atmosphere through
evaporation (Glushkov et al. 2005). Large shifts in CO2 concentrations in the oceans occurs
horizontally and vertically as a result of the slow rate of mixing by volume; the concentration of
dissolved CO2 is approximately 10 % higher by volume in the deep ocean than it is at the surface
(Sabine 2008).
Albedo
Albedo refers to the absorptive and reflectivity properties of clouds, the ocean and various
landforms to incoming solar radiation. Light colored surfaces such as snow reflect the greatest
amount of radiation back to space, whereas dark surface like asphalt absorb a lot of solar
radiation. Human land use practices affect earth’s albedo because development, deforestation,
desertification, agriculture and grazing livestock (a few of many human activities) change the
absorptive and reflective properties of earth’s surface. These activities therefore have a direct
affect on earth’s energy balance. Deforestation also affects the amount of vegetation available to
absorb CO2 and convert it to O2, through photosynthesis, which as described above, also affects
earth’s energy balance.
Different types of clouds have different physical properties which affect whether the cloud
absorbs or reflects short wave and long wave radiation. Stratocumulus clouds, which are low
thick clouds, cool the earth’s surface by reflecting short wave radiation back to space. In
contrast, high altitude cirrus clouds warm the atmosphere because they transmit incoming solar
radiation to earth’s surface and also reflect outgoing long wave radiation back to earth (NASA
2007). There is seasonal and regional variability in the cooling versus heating effect of clouds on
the global energy balance, and NASA scientists (2007) note that the effects of low and high
altitude clouds on climate generally balance each other out; the cooling effect of low altitude
clouds is slightly stronger than the warming effect of high altitude clouds, however (NASA
2007).
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Tectonics and Volcanism
Throughout earth’s history, levels of CO2 in the atmosphere has varied, ranging from over 3000
parts per million by volume (ppmv) to about 100 ppmv (Pagani et al. 2005). Extreme variations
in atmospheric CO2 have occurred in response to natural geologic and biological processes (e.g.,
Pearson and Palmer 2000; Berner and Kothavala 2001; Obzhirov et al. 2003; Cardellini et al.
2004; Pagani et al. 2005; Spence and Telmer 2005; Gurrieri et al. 2006). During the late
Paleocene and early Eocene, roughly 60 to 50 million years ago, atmospheric levels of CO2
ranged from 1000 to 1500 ppmv and during this period, temperate forests extended to the poles
and tropical climates extended to 45o N latitude (Pagani et al. 2005). Today only herbs, grasses,
forbs, sedges and stunted trees grow at high latitudes due to lower insolation levels, and arid
grasslands and temperate forests grow where tropical forests once thrived. The high levels of
atmospheric CO2 during this period are attributed to volcanism in East Greenland (Pagani et al.
2005) and potentially a massive release of methane from the disturbance of organic matter buried
on the sea floor as the result of an earthquake or mudslide (Venere 2006).
This period in earth’s geologic history is known as the Paleocene-Eocene Thermal Maximum
(PETM). The high CO2 levels of this geologic time in earth’s history, combined with increased
CO2 levels during the PETM led to acidification of the ocean, a 6o C to 7o C rise in high latitude
temperatures and contributed to the extinction of dinosaurs (Storey et al. 2007). Over the next
several million years, atmospheric CO2 gradually decreased with this trace gas reaching modern
levels by the late Oligocene (33.7 to 23.8 million years ago). Retallack et al. (2004: 817) note
that several factors may have contributed to this decrease in atmospheric CO2 including changes
in oceanic circulation associated with movement of continental plates, weathering associated
with mountain building, and the expansion of grassland and grazers into formerly forested areas.
Others note that a massive bloom of water ferns (Azolla) and subsequent die off resulted in a
drawdown of atmospheric CO2 from roughly 3000 ppmv to 650 ppmv, as the dead ferns sank to
the sea floor and became incorporated into deep sea sediments—known as the Azolla event
(Dickens et al. 1997; Pagani et al. 2005). The expansion of temperate forests during the Miocene
(23.03 to 5.33 million years ago) resulted in a further drawdown of atmospheric CO2 from 650
ppmv to 100 ppmv. After this period, earth’s plates continued to shift and mountains formed in
New Zealand and Europe affecting atmospheric and oceanic circulation. During the Miocene
earth began to experience ice ages, but the extreme glacial events of the Quaternary period
(starting 1.8 million years ago) would not occur for several million years. Atmospheric CO2 is
typically lower during glacial periods than during interglacial periods because ice sheets cover
areas that are blanketed with flora during interglacial periods.
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Shifts in the location of tectonic plates, affects atmospheric and oceanic circulation which affects
climate and the CO2 balance; small scale movements (earthquakes) also affect earth’s CO2
balance. Seismic slipping along fault lines can cause supersaturation of CO2 in the melted
sediment/rock. Infrared analysis of friction induced melts in rock, caused by seismic slipping
along the Nojima fault during the 1995 Kobe earthquake (Japan), indicate 1.8 to 3.4 thousand
tons of CO2 were released by the earthquake (Famin et al. 2007). Similarly, geochemical analysis
of water from springs located near active faults in the Gulf of Corinth, Greece (Pizzino et al.
2004) revealed high levels of dissolved CO2 for 1 to 10 months following earthquakes (Famin et
al. 2007).
Volcanism also affects the amount of CO2 in the atmosphere, but generally leads to hemispheric
cooling rather than heating because sulfur dioxide (SO2) is the primary gas released, not CO2
(Gerlach 1990, 1991; Halmer et al. 2002) (Figure 2). When Mount Pinatubo erupted in 1991, 14
to 26 million tons of SO2 were released to the atmosphere.
Figure 2. Satellite Photograph of an Exploding Volcano (from NOAA 2009a).
The SO2 combined with the haze created by the volcanic ash and dust cooled the atmosphere by
0.5oC for a period of 12 to 18 months, ameliorating any warming caused by emission of CO2 to
the atmosphere. However, active volcanic regions release CO2 to the atmosphere through
volcanic vents (fumaroles) and porous soil, even when the volcano is quiescent (USGS 2008).
For example, Ajuppa et al. (2004) studied rates of CO2 degassing on the flanks of the Somma-
Vesuvius volcano and found that soil CO2 concentrations ranged from 50 to 10,500 ppmv. In
another study, Favara et al. (2001) analyzed the amount of CO2 degassing from soils and vents
on Pantelleria Island, an active volcanic complex, to determine how much CO2 is emitted from
the soils, water and fumeroles on the island. These scientists found that 1.79 million metric tones
of CO2 was degassing from the soil, water and fumeroles on the island.
14
The emissions of SO2 and CO2 from terrestrial and marine volcanoes are significant sources of
trace gases into the atmosphere. Because of their threat to human life, as well as their impact on
climate, terrestrial volcanoes are extensively studied (USGS 2008). However, 70 % of
volcanic activity occurs along deep sea rifts located over one mile below the surface of the
ocean, and the effect these marine volcanoes have on earth’s climate is poorly understood
(NOAA 2009a). Because deep sea volcanoes have a significant impact on the global chemical
and heat balance, the NOAA established a program dedicated to studying deep sea hydrothermal
systems: Pacific Marine Environmental Laboratory (PMEL). In 2004, PMEL scientists studying
hydrothermal vents along the Mariana Arc in the North Pacific Ocean (Figure 3) discovered a
vent emitting a wide stream of effervescent bubbles (Lupton and Butterfield 2004). They
captured a sample of the liquid (Figure 4.) in containers and brought these to the surface for
analysis. Lupton and Butterfield (2004) identified 2.3 moles (101g) of gaseous CO2 per liter of
hot water recovered from the vent. The rate in which CO2 is released from one section of the
vent over a period of one day may be comparable to the rate of flow from a water hose. It is
estimated that 30 liters of water flows from an average backyard water hose (1.6 cm diameter)
every minute. If the amount of CO2 emitted from a 1.6 cm2 section of the hydrothermal vent was
constant for 24 hours this area would emit 4,300 metric tonnes of CO2 in one day. If a single 1.6
cm2 area of a vent released liquid CO2 year round, 9 million metric tonnes of CO2 would be
released from this small area in one year. Given there are almost 22,000 kilometers (~12,000
miles) of volcanic arcs along the ocean floor that are not well studied, this system could be
contributing significant levels of CO2 to the ocean and atmosphere.
Figure 3. Earth’s Plate Boundaries: The Mariana Arc (from NOAA 2009).
15
Figure 4. Photograph of Hydrothermal Vent Emitting Liquid CO2 (from NOAA 2009).
Atmospheric Circulation
The majority of the sun’s incoming solar radiation is received at the equator and this heat is
transported to the poles by atmospheric circulation. The Hadley cell (0 to 30o N/S), Ferrell cell
(30 to 60o N/S), and Polar cell (90 to 60o N/S) drive large scale atmospheric circulation and
distribute heat from the equator to the Poles (Figure 5). High pressure systems dominate the
Hadley cell between 20 and 40o N/S, and the Polar cell between 70 to 90o N/S. These systems
Figure 5. Schematic cross-section of earth’s atmospheric circulation cells.
16
form when dry air converges high in the atmosphere creating a parcel of air with higher pressure
than the surrounding atmosphere. The parcel of dry air sinks to earth’s surface creating some of
earth’s largest deserts. The Gobi (Asia), Great Victoria (Australia), Kalahari and Sahara (Africa)
and Sonoran (North America) occur in a band between 20 and 40o N/S. The Polar cell is also
comprised of dry air and as such the Arctic and Antarctic are considered polar deserts.
In contrast to areas of high pressure, low pressure systems dominate where moist air rises near
the equator and between 40 and 60o N/S. Low pressure systems form when air diverges in the
upper atmosphere creating a vacuum that draws in surface air. Air rushes in to fill the vacuum
created by a low pressure system. As the air rises it cools and condenses creating clouds and
precipitation. When extreme low pressure systems form over warm-ocean water the surrounding
air spirals in generating hurricanes and cyclones, such as hurricane Katrina (Handwerk 2005) and
tropical storm Kammuri (Bradhere 2008).
In addition to pressure (temperature) differences between the equator and poles driving
atmospheric circulation, physical forces associated with earth’s rotation on its axis affects
circulation. The force of earth spinning causes winds in the atmosphere to be deflected away
from the equator (Coriolis force). Winds associated with high pressure systems are deflected
clockwise in the Northern Hemisphere and counterclockwise in the Southern Hemisphere
(NASA 2007). Winds associated with low pressure systems are deflected counterclockwise in
the Northern Hemisphere and clockwise in the Southern Hemisphere. The Coriolis force also
results in the formation of earth’s prevailing winds: the Westerlies, Polar easterlies, Doldrums,
Horse latitudes and Trade Winds.
Intertropical Convergence Zone (ITCZ)
Seasonal changes in the location of the solar zenith effects shifts in the location of the Hadley,
Ferrell and Polar cells; the shift is greatest near the equator creating the Intertropical
Convergence Zone (ITCZ). The ITCZ is an area of low pressure that forms where the Northeast
Trade Winds meet the Southeast Trade Winds near the earth's equator. As these winds converge,
moist air is forced upward—as the air cools it condenses and creates a heavy band of
precipitation—the ITCZ also affects the duration and intensity of monsoon rains. In response to
changes in the location of the solar zenith, the ITCZ shifts from approximately 25 o N in
Northern Hemisphere summer (June-July-August) to 20o S in Southern Hemisphere summer
(November-December-January); the shift in the ITCZ results in monsoons in each hemisphere
(Gordon 2000).
17
Oceanic Circulation
Like the atmosphere, oceanic circulation distributes heat from the equator to high latitudes in
currents driven by earth’s prevailing winds, the Coriolis force and differences in the salinity
(density) of the water (Gross 1993). Because large scale ocean circulation is driven by
differences in temperature and salinity it is referred to as thermohaline circulation. The upper
400 meters of the ocean is also driven by prevailing winds in the atmosphere and wind driven
currents are critical to the movement of warm equatorial surface waters to higher latitudes
(Figure 6). The Gulf Stream, originating in the Gulf of Mexico is the largest surface current on
earth (NOAA 2009c). The Gulf Stream carries warm, relatively fresh water along the eastern
coast of North America to northern Newfoundland where it is deflected east by the Coriolis force
and flows to the mid-Atlantic ocean. West of Ireland, the current splits with one branch flowing
north and another south. The northern branch becomes a broad, shallow swath of warm water
called the North Atlantic Drift Current (NADC) which carries warm saline water to the North
Atlantic, moderating the climate of Europe and western Scandinavia. The southern branch of the
current joins the southward flowing Canary Current, which is wide, slow moving current that
flows south to Senegal where it is deflected west (Rossby 1996 and 1999).
Figure 6. Oceanic Circulation: Earth’s Thermohaline Belt (from NOAA,2009).
18
A similar circulation system occurs in the Pacific Ocean. The Kuroshio Current is akin to the
Gulf Stream, originating near Taiwan it flows north along the coast of Asia carrying warm water
to the North Pacific Ocean. The current is deflected west north of Japan and becomes a broad
swath of warm water moving east. In the eastern North Pacific Ocean the current splits into a
northern and southern branch. The northern branch, the Alaska Current carries warm waters
north and the southern branch, the California Current, carries cooler waters south.
The surface and deep water currents of the oceans form the Meridonal Overturning Circulation
(MOC) system. Surface currents are driven by wind, whereas deep ocean currents are driven by
differences in temperature and salinity. In the North Atlantic, the warm surface water condenses
when it encounters colder air causing seasonal fog, rain and snow in Europe and Scandinavia (a
similar system exists in the North Pacific Ocean). The colder, highly saline water left behind is
dense and sinks to depths of 1500 to 2500 m (4900 to 8200 ft), forming the North Atlantic Deep
Water (NADW) current. The NADW flows south along the coasts of the Americas finally
deflecting east near the tip of South America to join the Antarctic Circumpolar Current (ACC).
The ACC flows along the northern edge of Antarctica until it splits into two branches off the tip
of South Africa. One branch flows north into the Indian Ocean and another continues east along
the Antarctic coast until it reaches the Pacific Ocean. Here the current deflects and flows north
off the New Zealand coast and ultimately into the North Pacific Ocean (Smith et al. 2008).
In the North Pacific, this cold, deep current gradually mixes with overlying warmer surface water
and forms into a surface current deflected to the southwest and into the Indonesian Ocean. The
current continues a westward path, with branches entering the Indian and Atlantic oceans. As it
reaches the Atlantic Ocean, the current is deflected north and ultimately returns to the North
Atlantic Ocean where it once again mixes with cold, saline water, sinks and the conveyor-belt
cycle begins again. Oceanic models indicate it takes approximately 1000 years for a parcel of
water within the conveyor belt to complete one cycle from the North Atlantic Ocean to the North
Pacific Ocean and back to the North Atlantic Ocean (Doney et al. 2006).
Changes in Atmospheric and Oceanic Circulation
Changes in the volume and temperature of the Gulf Stream and Kuroshio Current can cause
significant changes in regional weather in the North Pacific Ocean and North Atlantic. Seasonal
changes in regional sea surface temperature as well as shifts in the location and intensity of
surface ocean currents and deep water upwelling cause changes in regional and global climate
(Broeker 1997; Little et al. 1997; Doney et al. 2006; Randall et al. 2007; NOAA 2009c). These
are referred to as coupled ocean-atmosphere circulation systems and shifts in these systems can
19
have dramatic effects on the intensity and duration of droughts in some regions and storms in
others. Systems that are tracked by NOAA include the: Pacific North American (PNA)
Oscillation, Arctic Oscillation (AO), North Atlantic Oscillation (NAO), El Nino/Southern
Oscillation (ENSO), and Antarctic Oscillation (AAO) (NOAA 2006b).
The location and intensity of weather patterns associated with each of these systems is driven by
the location and intensity of the high and low pressure systems that drive them (Randall et al.
2007; NOAA 2009b), as well as the influence of surface currents and NADW (Schiller et al.
1997; Bischoff et al. 2003). For example, the strength of the NAO is directly affected by the
warmth and volume of the Gulf Stream current (Saunders and Qian 2001; NOAA 2009b).
Variation in the NAO effects winter weather in Europe and the UK (Saunders and Qian 2002). A
moderately negative NAO leads to colder, drier, and calmer winters than average in northwest
Europe and warmer and wetter winters in southern Europe (Saunders and Qian 2001). A
moderately positive NAO results in wetter, stormy winters than average in northwest Europe,
and cold dry winters in southern Europe (Saunders and Qian 2001).
Like the NAO, variation in ENSO can significantly influence weather patterns in different
regions. Warm ENSO events (El Niño) occur when sea surface temperatures (SST) are
unusually warm in the central and east-central equatorial Pacific (Figure 7). El Niño events
typically result in above average precipitation in California and Mexico and drought in eastern
Australia (NOAA 2009b). Cool ENSO events (La Niña) occur when SST in the equatorial
pacific are unusually cool and result in above average precipitation in the Northwest of North
America, dry conditions in California and Mexico and increased rains in eastern Australia
(NOAA 2009b).
Figure 7. El Niño Southern Oscillation: El Niño and La Niña (from NOAA 2009b).
20
Temporal Variations in Atmospheric and Oceanic Circulation
Changes in atmospheric and oceanic circulation driven by low frequency changes in earth orbit
around the sun (celestial mechanics: see below) contributed to earth’s glacial and interglacial
periods. Little et al. (1997) speculated that at different times in the past, intensified trade winds,
forced a higher volume of warm tropical and subtropical waters across the equator and into the
Gulf Stream. As this large body of warm water moved into the North Atlantic it cooled and
condensed resulting in increased precipitation/ snow, enhancing the growth of ice-sheets and
potentially contributing to the onset of ice ages (Broecker 1997; Little et al. 1997;; Clark et al.
2002; Manabe and Stouffer 1988, 1997; Manabe et al. 1991; Vellinga and Wood 2002;
Stoufferand Manabe 2003). Near the end of interglacial periods, it is conceivable that heat
stored in the atmosphere and ocean over thousands of years drives more intensive tropical and
subtropical storms resulting in more fresh water being dumped into the Gulf Stream through
runoff and precipitation (Douglas 1989). Over several years, the repeated influx of low-saline
water from the Gulf Stream into the Atlantic Ocean would dilute the cold, high-saline Arctic
waters, potentially causing the MOC to shut down (Douglas 1989). Shutting down the MOC
would cause water from the Gulf Stream to pool in the North Atlantic, causing higher levels of
precipitation and stronger storms in Western Europe and Scandinavia. This precipitation and
cooler temperatures would enhance the growth of alpine glaciers and ice sheets in these regions.
Additionally, because fresh water freezes at a higher temperature than salt water 0o C versus -1.9o
C to -19o C, respectively (the temperature at which sea water freezes varies considerably,
contingent upon the level of salinity, wind sheer, current strength), sea ice could form more
readily as a result of an influx of less saline water to the Arctic via the Gulf Stream (see for
example Frey et al. 2003).
Celestial Mechanics
The astronomical theory developed by Milutin Milankovitch in the early 1900s is widely
accepted by climate scientists as the best theory for explaining changes in the seasons, as well as
climate change over hundreds of thousands of years (Milankovitch 1941; Kerr 1987).
Milankovitch identified seasonal and longer-term systematic variations in earth’s orbit around
the sun based on meticulous measurements on the position of stars and equations that explained
how the gravitational pull of other planets and stars affected earth’s orbit. Through his
calculations, Milankovitch identified three primary celestial mechanisms that affect long-term
cycles of cooling and warming on earth including eccentricity, precession of the equinox and
obliquity. Each of these is discussed in greater detail below.
21
Eccentricity refers to a systematic shift in earth’s orbit around the sun from an eclipse to a
circular pattern and back to an eclipse every 95,000 to 136,000 years, averaging 100,000 years
(Figures 8 and 9). The shape of earth’s orbit around the sun affects how close the earth is to the
Figure 8. Schematic of Variation in Earth’s Axial Tilt (from NOAA 2009).
23
sun on its annual cycle. When earth’s orbit is circular, its distance from the sun is relatively
steady throughout the year, minimizing extreme seasonal variation. When earth’s orbit is
eccentric, seasonal variation in temperature is more extreme. In an eccentric orbit, the earth is
closest to the sun at perihelion and farthest from the sun at aphelion. If perihelion occurs during
northern hemisphere summer this accentuates the length and intensity of the summer season. If
aphelion occurs during northern hemisphere summer, the season is shorter and less intense.
Precession refers to a wobble of the earth in its orbital path around the sun that occurs every
19,000 to 23,000 years (refer to Figure 9). This wobble affects the point when earth’s orbit is
nearest the sun (the location of perihelion), and shifts from the northern to the southern
hemisphere approximately every 9,500 to 11,500 years. Changes in earth’s orbital cycle
(eccentric or round) accentuate the affect of precession on hemispheric warming and cooling
(Imbrie and Imbrie 1980; Bradley 1985; Kutzbach 1987).
Obliquity refers to the earth rotating on an axis that is tilted at an oblique angle to the plane of
ecliptic (Figure 9); the angle of earth’s tilt varies from 22.3 to 24.5o every 41,000 years. This tilt
is what causes the seasons; northern hemisphere summer occurs when the North Pole is tilted
toward the sun, and southern hemisphere summer occurs when the South Pole is tilted toward the
sun. Seasons can be accentuated or modified by eccentricity and precession.
Astronomical theory suggests that cyclic changes in earth’s orbital parameters accentuates
seasons and contributes to the onset of glacial and interglacial periods. Examination of the
mathematical components of eccentricity, obliquity and precession reveal several components
that suggest periodic movement of a wave in a fixed frequency and wavelength (Imbrie and
Imbrie 1980). As such, changes in earth’s orbital parameters can be calculated over the past
several million years as well as into the future (Imbrie and Imbrie 1980). The mathematical
certainty of earth’s orbital parameters allows climate scientists to use the calculations to
reconstruct the timing of glacial and interglacial periods, as well as predict future climate driven
by celestial mechanics (e.g., Ruddiman et al. 2005; Douglas 2007a and 2007b; Stuckless and
Levitch 2007) (Figure 10). However, Imbrie and Imbrie (1980) caution that celestial mechanics
explain only 25% of climate change, noting that other natural forcing mechanisms and feedbacks
drive 75 % of climate change.
24
Figure 10. Reconstruction of Insolation (400,000 years to present) based on Earth’s Orbital Parameters (from NOAA 2009).
Climate Models Over the past thirty years, scientists have developed models to simulate changes in earth’s
climate on global (Muller 1997; Muller et al. 1997; Lopez et al. 2006), hemispheric (Kutzbach
1987) and regional scales (Giorgi and Francisco 2000a and 2000b), based on celestial mechanics
and other natural forcing mechanisms. Models utilized by climate scientists vary in their
resolution and sophistication. Common models used to better understand past glacial and
interglacial periods as well as predict future climate include: earth system models of intermediate
complexity (EMICs), general circulation models (GCMs), and atmospheric-ocean general
circulation models (AOGCM) (see Figures 11, 12 and 13 for images of climate models) (Randall
et al. 2007).
Climate models are based on the fundamental laws of physics, such as Fourier’s law of heat
conduction (heat moves matter (or air) from an area of higher temperature to an area of lower
temperature), or Newton’s laws of motion (Randall et al. 2007). To simulate climate, scientists
must enter specific boundary conditions into their models including solar radiation at the top of
the atmosphere, composition of the atmosphere, height of the land surface including mountains
and ice sheets as well as the characteristics of these landmasses (e.g. albedo and roughness)
(Kutzbach, 1987). Sea-ice location, extent of the ocean surface and ocean temperature and
locations of other major water bodies (such as the Great Lakes) are also crucial variables.
Provided this information is correct, GCMs and AOGCMs can simulate many (but not all)
features of the present climate (Randall et al. 2007). Changes in any one of these systems effects
changes in the others.
25
Figure 11. 3-D Image of a Climate Model: Atmosphere and Ocean (from NOAA 2009).
Figure 12. 3-D Image of a Climate Model of Hurricane Katrina (from NOAA 2009).
26
Figure 13. 3-D Image of a Climate Model: Atmosphere and Ocean (from NOAA 2009).
The IPCC Climate Models The EMICs used by the IPCC were developed specifically to investigate physical processes and
interactions within the climate system over long time scales. EMICs are more simplistic models
than AOGCMs, but because they simulate fewer complex variables they require less computer
time. The time required to run different types of climate models is critical because few
computers in the world have the capacity to run AOGCMs and model run-times on these
computers are costly and therefore limited (Randall et al. 2007). EMICs therefore compliment
AOGCMs, providing inferences about large scale processes over longer periods of time than can
be achieved by current AOGCMs (Randall et al. 2007:592).
Scientists contributing to the IPCC Fourth Annual Report analyzed 22 AOGCMs developed by
leading research institutes in Australia, Canada, China, France, Germany, Japan, Korea, Norway,
Russia and the United States (Randall et al. 2007). A summary of the parameters included in a
selection of the models analyzed by the IPCC is provided in Appendix 1 Model Parameters. For
detailed information on the variables and parameters of these AOGCMs please refer to Randall
et al. (2007:597-599). In general, the AOGCMs utilized by the IPCC varied in sophistication as
determined by their horizontal and vertical resolution, as well as the complexity of physical
27
dynamics and feedbacks modeled. Horizontal resolution in the AOGCMs varied from 1o x 1o of
longitude and latitude to 4o x 5 o longitude and latitude. Similarly, there was variability in the
height of the atmosphere modeled above the ground surface (2500 pascals to 5 pascals [25 mbar
to 0.05 mbar]) as well as how the atmosphere was subdivided into different levels, ranging from
16 to 56 levels. Similarly, the horizontal resolution of the ocean grid varied (0.2° x 0.3° to 4 o x
5 o) as did ocean flow (rigid lid to a free surface), and depth (16 to 45 levels) below surface.
The characteristics of sea ice dynamics and structure also varied in the AOGCMs with some
scientist’s modeling the physical/elastic properties of sea ice as it interacts with the atmosphere,
ocean and other sea ice. Other models were simpler and did not calculate the dynamics of these
physical interactions; rather they assumed free drift of the sea ice. There was also a range of
variability in how land features were modeled with some representing soil moisture as a single
layer and others as multiple layers; the extent and complexity of the vegetation canopy and river
routing also varied between models. The IPCC climatologists also note whether they made
adjustments for surface momentum, and heat or freshwater fluxes in coupling the atmosphere,
ocean and sea ice components of the models (Randall et al. 2007:597). Below, the potential
future climate scenarios predicted by these models are compared with simulations of climate
conditions during the last interglacial period. These comparisons are made to determine how
warmer temperatures than present affected the earth’s environment.
Climate Models of the Past for Predicting the Futur e
Kaspar and Cubasch (2006) used a coupled AOGCM called ECHO-G to analyze how changes in
Earth’s orbital parameters influenced the last interglacial (Eemian) and subsequent glacial epoch.
Their model determined that temperatures in the Arctic were approximately 4oC warmer than
present (Kaspar and Cubasch 2006). Astronomical models of earth’s orbital parameters for the
period spanning 130,000 to 125,000 years ago, suggest that summers were considerably warmer
than today because earth’s axial tilt was more extreme than today (Kaspar and Cubasch 2006).
Further, during this period earth’s precession was at perihelion during northern hemisphere
summer, magnifying the effect of earth’s extreme tilt on the amount of solar radiation received in
the Arctic. Paleoenvironmental studies (discussed in greater detail in a later section of this
paper), indicate that during the Eemian interglacial (ca. 130,000 – 115,000 years ago), ice sheets
were significantly smaller (Cuffey and Marshall, 2000; Tarasov and Peltier, 2003; Lhomme et al.
2005), and sea level was 4 to 6 m (13 to 20 ft) higher than it is today (Scherer et al. 1998;
Shackleton et al. 2002; Overpeck et al. 2006).
28
Within the first few thousand years of the onset of the Holocene interglacial (roughly 9,000 to
8,000 years ago), earth’s orbital parameters were similar to those calculated for the Eemian
(Bradley 1980; Kutzbach 1987; Lorenz et al. 2006). Correspondingly, summer insolation and
temperatures in the northern hemisphere were higher than they are at present (Lorenz et al.
2006). Since that time, earth’s tilt has become less extreme and perihelion shifted from summer
to spring 5,500 years ago and now occurs during winter (refer to Figure 9) (Bradley 1985). This
orbital cycle is similar to that of the Eemian: The most extreme orbital parameters occurred
within the first few thousand years of the onset of the interglacial, and over the next 10,000 years
earth moved into a glacial period. Astronomical models indicate earth is currently moving into a
glacial epoch, but one that is not as extreme or as cold as the last glacial epoch (Ruddiman et al.
2005; Douglas 2007a and 2007b; Stuckless and Levitch 2007). Some climate scientists speculate
that current and estimated future levels of anthropogenic GHG emissions in the atmosphere will
keep earth from moving into an ice age (Jansen et al. 2007; Randall et al. 2007).
Climate models evaluated by the IPCC Fourth Working Group suggest that by 2090
anthropogenic GHG emissions will not only stop the next ice age, but will override the global
cooling being driven by celestial mechanics (Allali et al. 2007; Randall et al. 2007).
Anthropogenic GHG emissions will amplify the greenhouse effect and cause global temperatures
to rise resulting in environmental conditions similar to those of the Eemian interglacial. The
Fourth Working Group modeled future climate based on seven different social, technological and
economic scenarios that represented potential energy use and land use practices in different
regions of the world. Simulations of the most conservative scenarios indicate that by 2090-2099,
northern hemisphere temperature will rise less than 2oC, and sea level will rise less than 10
centimeters (Table 1). Simulations of more extreme scenarios suggest northern hemisphere
temperature will rise by up to 6.4oC, global temperature will increase an additional 2oC and sea
level will rise up to 0.59 m by 2090-2099 (Jansen et al. 2007; Randall et al. 2007).
The IPCC Fourth Working Group models suggest that by 2300, global warming induced by
anthropogenic GHG emissions will cause the Arctic ice pack and the Greenland ice sheet to melt,
sea level will rise 5 m above its present elevation and the MOC will shut down (Randall et al.
2007).
29
Table 1. IPCC CO2-eq Social, Economic and Technological Scenarios and Their Impacts, 2090-2099
Scenarios GHG
Equivalent (ppm) Likely Temp Increase ( C )
Range of Temp Increase ( C )
Estimated Sea Level Rise
B1 Scenario 600 1.8 1.1-2.9 0.18-0.38 A1T Scenario 700 2.4 1.4-3.8 0.2-0.45
B2 Scenario 800 2.4 1.4-3.8 0.2-0.43 A1B Scenario 850 2.8 1.7-4.4 0.21-0.48
A2 Scenario 1250 3.4 2.0-5.4 0.23-0.51 A1F1 Scenario 1550 4 2.4-6.4 0.26-0.59 Scenario Descriptions
A1 Scenario Split into three sub-scenarios -- assumes world with very rapid global population Rapid introduction of more efficient technologies growth that peaks around 2050.
A1T Scenario Adopts non-fossil energy technologies A1B Scenario Balanced adoption of technologies (fossil and non-fossil)
A1F1 Scenario Fossil intensive technologies A2 Scenario A heterogenous world with high population growth, slow economic development and slow
technological change B1 Scenario Same population as A1 scenario, but more rapid changes toward a service and information
economy B2 Scenario Intermediate population with emphasis on local solutions to economic, social and
environmental solutions
Oceanic models indicate the MOC could shut down if a large enough flux of fresh water entered
the Arctic Ocean when the Greenland ice sheet melted, because the salinity and density of North
Atlantic waters would be reduced and the NADW current would not be able to form (e.g.
Broecker 1997; Clark et al. 2002; Manabe and Stouffer1988, 1997; Vellinga and Wood 2002).
For example, climate models and paleoenvironmental reconstructions (see next section) indicate
that the MOC shut down between 12,800 and 11,000 years ago following a catastrophic release
of fresh water into the North Atlantic from Lake Agassiz, a glacial lake spanning the borders of
Manitoba, North Dakota and Minnesota (Broecker 2003). When glacial ice receded at the end of
the last ice age, Lake Agassiz flooded the Mississippi drainage and St. Lawrence Valley and the
cold glacial water flowed to the Atlantic Ocean causing rapid cooling of the northern
Hemisphere; this period is referred to as the Younger Dryas (Dansgaard et al. 1989; Broecker
1997; Clark et al. 2002).
IPCC and Ocean Acidity
In addition to modeling the effect of anthropogenic GHG emissions on climate change, IPCC
also evaluated models that examine the effect of these emissions on ocean acidity (Meehl et al.
2007). When CO2 enters the ocean it is converted to carbonic acid and bicarbonate and carbonate
ions resulting in a reduction in the pCO2 in the water which facilitates diffusion of more CO2
from the atmosphere (Sabine 2008). Recent studies indicate that increases in anthropogenic
30
atmospheric CO2 are causing more CO2 to be absorbed by the ocean. Correspondingly, the ocean
is becoming more acidic which is dissolving the shells of marine organisms, killing plankton,
reducing the number of organisms that absorb CO2, and throwing the marine ecosystem off
balance (Allali et al. 2007; Meehl et al. 2007).
Verifying Climate Models Predicting earth’s future climate is strongly dependent on the assumptions underlying the
methods used in the models (Lopez et al. 2006) and the current state of scientific understanding
of climate dynamics (Kettleborough et al. 2006). In the 1980s, leading climate scientists noted
that models only predicted future climate with about 25% accuracy (Imbrie and Imbrie 1980).
Fortunately, since that time the accuracy and reliability of climate models has enhanced
significantly. Given the importance of climate models in estimating the impacts of anthropogenic
GHG emissions and land use practices on global warming, scientists have devoted considerable
effort to enhancing the reliability of climate models. The most critical measure of a climate
model’s ability to predict climate is its ability to reliably reconstruct climate for a period of
historic record.
Nine AOGCMs used by the IPCC Third Working Group were independently evaluated by Girogi
and Mearns (2001) to determine their accuracy and reliability simulating climate for two of the
IPCC’s forcing scenarios (A2 and B2, see above). The A2 scenario developed by the IPCC is
considered to have ‘high’ GHG forcing and the B2 scenario is considered to have ‘medium low’
GHG forcing. Statistical analyses of the nine models were performed to calculate the reliability
of their estimates of temperature and precipitation for 22 land regions around the world for the
period spanning 1961-1990 (Giorgi and Mearns 2001:1144). The results were compared to
historical records to determine the reliability of each model. Following this, they performed
statistical analyses to evaluate the temperature and precipitation estimates derived from each
AOGCM against the other eight AOGCMs. They found that greater reliability could be obtained
by measuring the range of uncertainty in each model, and eliminating models that exceeded the
confidence interval of the other models (Giorgi and Mearns 2001:1143).
In their statistical evaluation of the AOGCMs, Giorgi and Mearns (2001) found that model
reliability ranged from 20 to 80% in their estimates of temperature, and 70 to 90% in their
estimates of precipitation. Based on their study, Giorgi and Mearns (2001:1155) recommended
that models should be tuned as accurately as possible to replicate present-day regional climate
conditions before being used to predict future climate. Several others have used similar
techniques to test the validity and reliability of climate models with similar results (see for
example Murphy et al. 2004; Piani et al., 2005; Shukla et al. 2006; Knutti et al. 2006).
31
Climate scientists contributing to the IPCC Fourth Working Group recognized that there was
considerable uncertainty in the models used by the Third Working Group, and as such
established 18 modeling groups that worked together to compare the accuracy and reliability of
the AOGCMs to be used by the Fourth Working Group (Randall et al. 2007). They performed
coordinated, standard modeling experiments and analyzed the results. These coordinated efforts
facilitated “rapid identification and correction of errors, the creation of standardized benchmark
calculations and a more complete and systematic record of modeling progress” (Randall et al.
2007:593). Accuracy and reliability of the AOGCMs was evaluated by forecasting weather for a
few days to a few months and comparing the model results with recorded climate data. The
Fourth Working Group enhanced the AOGCMs by reformulating energy transport schemes,
increasing the horizontal and vertical resolution of the models, and developing a more
comprehensive model of earth’s physical processes. The revised models predicted daily and
seasonal weather conditions with enough accuracy that they were determined capable of
simulating some key physical processes and teleconnections in the climate system (Randall et al.
2007:593).
The terrestrial and oceanic components of AOGCMs continue to be improved through systematic
evaluation of the models against actual observations, as well as against more comprehensive
models (Randall 2007:593). Terrestrial components critical to simulating large-scale climate
processes over the next 20 to 30 years are included in current AOGCMs, but these models do not
include physical dynamics that drive climate change on longer time scales (Randall et al. 2007).
Additionally, many AOGCMs still require significant advances to reliably model glacial and ice
sheet dynamics under the IPCC climate scenarios. Few AOGCMs include ice sheet and glacier
dynamics because several variables effect accumulation and ablation (melting/calving),
including: altitude, latitude, aspect, and distance from large water bodies. Greater progress has
been made modeling sea ice dynamics including consideration of sea ice thickness and
thermodynamics (including sea ice interface with underlying sea water and overlying
atmosphere). It is also difficult to model dynamics caused by freshwater fluxes such as river and
estuary mixing schemes, however, some AOGCMs include these variables (Randall et al. 2007).
Trace gases found in the atmosphere have also been incorporated into some models via
interactive aerosol modules, facilitating comparisons of predicted natural variation with
estimates of climate change under anthropogenic GHG driven scenarios (Forster et al. 2007;
Randall et al. 2007). For detailed information on models used by the IPCC Fourth Working
Group, refer to Randall et al. (2007).
Despite advances in AOGCMs, the Fourth Working Group identified several variables and
parameters that current models cannot estimate with reliability (Tables 2 and 3). In part, a
32
weakness of current AOGCMs is that they only model changes in solar radiation (as associated
with celestial mechanics) and volcanism as the only natural forcing mechanisms in climate
change: The other forcing mechanisms in the models are attributed to human land use practices
and anthropogenic GHG emissions. Given the complexity of earth’s physical systems and lag
time associated with the transport of heat energy and trace gases in the ocean, considerable work
is required to enhance AOGCMs so they can reliably simulate these systems over longer periods
of time (Table 4).
Reconstructing Past Environments to Predict the Fut ure
In order to understand the implications of how future climate change may affect life on earth,
scientist must reconstruct environments that existed in the past under different climatic
conditions. Using celestial mechanics as the primary forcing mechanism, climate scientists have
reconstructed the extent of glaciers and ice sheets at different times in prehistory (see for
example Ruddiman and Wright 1987), as well as estimated temperature and precipitation for
these periods. The accuracy of these models is verified through an examination of proxy data
(such as ancient pollen and microorganisms) recovered from sediment cores (Mix and Ruddiman
1984; Mix 1987; Bond et al. 1993; Williams et al. 1993), or oxygen and carbon isotopes
recovered from ice cores (Bender et al. 1994; Petit et al. 2000). Proxy data are used under the
principle of uniformatarianism, which postulates that the relationships between climatic
conditions and environmental response (e.g. precipitation, temperature and days of sunshine
required to grow certain species of plants) have operated unchanged throughout the period of
interest (Bradley 1980; Williams et al. 1993).
Proxy Data Proxy data commonly used to estimate past climatic conditions include: coral reefs, sediment
cores from lakes (sedimentological, isotopic, geochemical, and palynolgical analyses), ice cores
(isotopic and geochemical analyses), deep sea marine sediment cores (sedimentological, isotopic,
geochemical, and foraminiferal analyses), glacial geologic features, macrobotanical materials
(e.g., seeds, needles, twigs, cones), faunal materials, paleontological materials (fossilized animals
and plants) and tree-rings (Bradley 1985; Williams 1993). Each of these have different levels of
temporal and spatial resolution with tree-rings providing the highest level of resolution (seasonal
to annual resolution spanning several hundreds to several thousand years (e.g. Fritts 1976; Briffa
et al. 1990; Hughes 1991; Graumlich 1993; Douglas 1998) to oxygen isotopes (18O/16O ratios)
and hydrogen isotopes (2H) having the greatest spatial (global) and temporal resolution
(hundreds of thousands of years) (e.g. Mix 1987; Ruddiman 1987; Waelbroeck et al. 1995).
Below, the methods for reconstructing climate using pollen, macrobotanical materials and
isotopes are discussed.
33
Table 2. Sample of Data Gaps and Modeling Inadequacies Noted in IPCC Fourth Assessment Technical Reports (Randall et al. 2007 and Meehl et al. 2007)
For Clouds For Soil Moisture and Terrestrial Ice For Sea Ice Nevertheless, important deficiencies remain in the simulation of clouds and tropical precipitation (with their important regional and global impacts) (Randall et al. 2007:592)
Overall, the uncertainty in surface-atmosphere coupling has implications for the reliability of the simulated soil moisture atmosphere feedback. It tempers our interpretation of the response of the hydrologic cycle to simulated climate change in ‘hot spot’ regions. Note that no assessment has been attempted for seasons other than NH summer (Randall et al. 2007: 606).
Despite notable progress in improving sea ice formulations, AOGCMs have typically achieved only modest progress in simulations of observed sea ice since the TAR. The relatively slow progress can partially be explained by the fact that improving sea ice simulation requires improvements in both the atmosphere and ocean components in addition to the sea ice component itself (Randall et al. 2007: 592)
The relatively poor simulation of these clouds in the present climate is a reason for some concern. The response to global warming of deep convective clouds is also a substantial source of uncertainty in projections since current models predict different responses of these clouds. Observationally based evaluation of cloud feedbacks indicates that climate models exhibit different strengths and weaknesses, and it is not yet possible to determine which estimates of the climate change cloud feedbacks are the most reliable (Randall et al. 2007:593)
Evaluation of the land surface component in coupled models is severely limited by the lack of suitable observations. The terrestrial surface plays key climatic roles in influencing the partitioning of available energy between sensible and latent heat fluxes, determining whether water drains or remains available for evaporation, determining the surface albedo and whether snow melts or remains frozen, and influencing surface fluxes of carbon and momentum. Few of these can be evaluated at large spatial or long temporal scales. This section therefore evaluates those quantities for which some observational data exist (Randall et al. 2007: 617).
Additionally, while impressive advances have occurred in developing sea ice components of the AOGCMs since the TAR, particularly by the inclusion of more sophisticated dynamics in most of them (see Section 8.2.4), evaluation of cryospheric feedbacks through the testing of model parametrizations against observations is hampered by the scarcity of observational data in the polar regions. In particular, the lack (Randall et al. 2007: 639)
Significant uncertainties, in particular, are associated with the representation of clouds, and in the resulting cloud responses to climate change. Consequently, models continue to display a substantial range of global temperature change in response to specified greenhouse gas forcing (Randall et al. 2007:601)
Because the available models do not include all relevant processes, there is much uncertainty and no consensus about what dynamical changes could occur in the Antarctic Ice Sheet (see, e.g., Vaughan and Spouge, 2002; Alley et al., 2005a). Paleoclimatic data indicate sea level was 4 to 6 m higher than present during the last interglacial, and these levels cannot be explained by a reduction in the Greenland ice sheet. As such, Oppenheimer and Alley (2005) speculate that an increase of 2°C in global temperature is the threshold beyond which the West Antarctic Ice Sheet will melt and contribute to sea level rise (Meehl et al. 2007: 831).
In general, the possible climate changes associated with future evolution of the Greenland Ice Sheet are better understood than are those associated with changes in the Antarctic Ice Sheets (Randall et al. 2007: 642)
34
Table 3. Sample of Data Gaps and Modeling Inadequacies Noted in IPCC Fourth Assessment Technical Reports (Forster et al. 2007 and Meehl et al. 2007)
For Aerosols and Water Vapor
For dates before about 1950 indirect measurements are relied upon. For these periods, levels of atmospheric CO2 are usually determined from analyses of air bubbles trapped in polar ice cores. (Forster et al. 2007:137)
One of the large sources of uncer-tainties is the poor knowledge of the amount and distribution of anthro-pogenic aerosols used in the model simulations, particularly for pre-industrial conditions (Forster et al. 2007:179)
Some effects are not quantified, either because they do not have enough evidence or because their quantification lacks consensus. These include certain mechanisms associated with land use, stratospheric water vapour and cosmic rays (Forster et al. 2007:200).
Since the AOGCMs are integrated with scenarios of CO2 concentration, uncertainties in carbon cycle feedbacks are not included in the results. The carbon cycle uncertainty in projections of temperature change cannot be translated into sea level rise because thermal expansion is a major contributor…” (Meehl et al. 2007: 820)
Models also have weaknesses in representing convection processes and aerosol distributions, and simulating updraft velocities and convection-cloud interactions. Even without considering the existing biases in the model-generated clouds, differences in the aerosol chemical composition and the subsequent treatment of activation lead to uncertainties that are difficult to quantify and assess. The presence of organic carbon, owing to its distinct hygroscopic and absorption properties, can be particularly important for the cloud albedo effect in the tropics (Ming et al., 2007). (In Forster et al. 007:179)
Uncertainties in the water vapour flow to the atmosphere from irrigation are significant and Gordon et al.(2005) gave a substantially higher estimate compared to that of Boucher et al. (2004). Most of this uncertainty is likely to be linked to differences between the total withdrawal for irrigation and the amount actually used (Boucher et al., 2004). Furthermore, Gordon et al. (2005) also estimated a reduced water vapour flow to the atmosphere from deforestation, most importantly in tropical areas. This reduced water vapour flow is a factor of three larger than the water vapour increase due to irrigation in Boucher et al. (2004), but so far there are no estimates of the effect of this on the water vapour content of the atmosphere and its RF. Water vapour changes from deforestation will, like irrigation, affect the surface evaporation and temperature and the water cycle in the atmosphere. Radiative forcing from anthropogenic sources of tropospheric water vapour is not evaluated here, since these sources affect surface temperature more significantly through these non-radiative processes, and a strict use of the RF is problematic. The emission of water vapour from fossil fuel combustion is significantly lower than the emission from changes in land use (Boucher et al., 2004). (In Forster et al. 2007:185)
Testing the reliability of estimates of radiative forcing caused by GHGs and ozone is difficult due to the lack of high resolution historical data as well as uncertainties in the knowledge of past emissions and chemical-microphysical modeling. (Forster et al. 2007:208).
35
Tree Rings as Proxy Data
Tree growth is constrained by available water and temperature, and different species of trees are
either more sensitive to shortages of water or extreme heat. Trees that are constrained by
available water grow less during drought years, such as Piñon pine (Pinus edulis), and this is
reflected in their annual growth rings. Trees that are constrained by temperature at high
elevations, such as Bristlecone pine (Pinus aristata and Pinus longaeva), grow less during short
summer seasons (Figure 14). By correlating the annual growth rings (Figure 15) of several trees
growing in an area, dendrochronologists develop a tree-ring chronology that reflects the average
response of trees growing at that site to either temperature or precipitation (see Fritts 1970). As
such, through statistical analyses annual tree rings can be used to reconstruct climate for the
length of the tree-ring chronology. For example, the Bristlecone pine chronology for the White
Mountains, California has been used to reconstruct temperature going back over 7,000 years
(LaMarche 1973).
Figure 14. Photograph of Bristlecone Pine Tree from White Mountains (NOAA 2009).
Figure 15. Image of Tree-rings for Reconstructing Climate (NOAA 2009).
Table 4. Climate Models and Their Evaluation (after Randall et al. 2007)
Quote from Randall et al. (2007:601) Quote from Randall et al. (2007:602)
Deficiencies remain in the simulation of tropical precipitation, the El Niño-Southern Oscillation and the Madden-Julian Oscillation (an observed variation in tropical winds and rainfall with a time scale of 30 to 90 days). The ultimate source of most such errors is that many important small-scale processes cannot be represented explicitly in models, and so must be included in approximate form as they interact with larger-scale features. This is partly due to limitations in computing power, but also results from limitations in scientific understanding or in the availability of detailed observations of some physical processes.
The climate system includes a variety of physical processes, such as cloud processes, radiative processes and boundary-layer processes, which interact with each other on many temporal and spatial scales. Due to the limited resolutions of the models, many of these processes are not resolved adequately by the model grid and must therefore be parametrized. The differences between parametrizations are an important reason why climate model results differ.
36
Pollen as Proxy Data
All plants, trees and grasses have temperature and precipitation thresholds that constrain where
they can grow; soil type and amount of sunlight also affect growth. As such, pollen can be used
to reconstruct the climate at the time the plant, tree, or grass lived. Several studies have been
done to identify how far different types of pollen can be transported on the wind (e.g. Jansson
1966, 1973; Barnosky et al. 1987; Jacobsen et al. 1987; Bradley 1995). Pollen grains of
flowering plants are relatively heavy and sticky and are either transported by insects or fall near
the plant (Figure 17). In contrast, pollen of non-flowering plants and trees (e.g. pines, firs and
spruce) are winged so that they can be transported great distances on the wind. Differences in
how pollen of different species are transported facilitates reconstructions of local (flowering) and
regional (non-flowering) shifts in vegetation over time based on pollen recovered from sediment
cores (e.g. Barnosky et al. 1987; Jacobsen et al. 1987).
Figure 16. Pollen grains (from www.vancouver.wsu.edu)
Macrobotanical Materials as Proxy Data
Like the pollen of flowering plants, macrobotanical remains (e.g. seeds) are not transported far
by wind. However, seeds and other macrobotanical materials are often deposited in lake or bog
sediments and can be used to reconstruct the environment, temperature and precipitation that
existed locally at the time that they were deposited. Macrobotanical materials can also be
recovered from packrat middens and used to reconstruct the habitat surrounding the midden
(Figure 17).
37
Figure 17. Paul Martin and an indurated packrat midden (from NOAA 2009).
Packrats are medium-sized rodents (Figure 18) and live in a range of habitats from sea level to
approximately 3,350 m (10,988 ft) elevation. Packrats collect various plant materials within 30 to
50 m (100 to 165 ft) of their den for food as well as to construct a nest (Betancourt et al. 1990).
These materials can be preserved for several thousand years when they are deposited in the right
setting and conditions (Van Devender et al. 1987). When packrats create dens in dry
rockshelters, portions of their dens can become indurated by urine and form into hard, dark
organic deposits termed middens. These middens can provide a rich source of well preserved,
perishable organic materials from deserts, woodlands, and forests that represent a “snap shot” of
the habitat that existed when the den was created (Betancourt et al. 1990). Plant materials
recovered from middens can typically be identified to species and radiocarbon dated with great
enough accuracy to establish a date of deposition with a standard deviation of only +/- 50 to +/-
150 years. By analyzing middens from different elevations that date to approximately the same
period it is possible to reconstruct a “habitat” transect for a specific period.
Figure 18. Photograph of a Packrat (from NOAA 2009).
38
Isotopes as Proxy Data
Reconstructions of global-scale climate change are derived from oxygen, carbon and hydrogen
isotopes recovered from foraminifera and ice cores. Foraminifera are single-cell organisms that
range in size from 100 micrometers to 20 cm in length (Figure 19). These organisms form shells
made of CaCO3; the oxygen in these shells is comprised of two different isotopes (18O and 16O),
the ratio of these isotopes present in an organism provide a signature of global ice volume and
temperature of the ocean where the organism lived. The 16O isotope is lighter than the 18O
isotope and therefore evaporates more readily from oceans and other water bodies. During an
interglacial, these isotopes readily re-enter the ocean or other water body through a cycle of
evaporation/ condensation and rain. In contrast, during glacial periods the 16O becomes trapped
in polar ice essentially removing it from the evaporation/ condensation cycle. These physical
dynamics result in changes in the 18/16O ratio present in the shells of foraminifera (and ice cores)
during glacial and interglacial periods—the ratio of 18/16O is referred to as the delta and is
hereafter shown as δ 18O.
Figure 19. Photograph of a Foraminifera (from NOAA 2009).
Some of the earliest work on δ18O was conducted by Emiliani (1955) who extracted oxygen
isotopes from foraminifera recovered from marine sediment cores, and recognized that they
could be used as a paleothermometer. Although there is still some controversy over the rates,
timing and nature of conditions under which planktonic (shallow) versus benthic (deep sea)
foraminifera shells calcify (affecting the δ18O signature) most oceanographers and climate
scientists recognize that there is a remarkable similarity among planktonic and benthic δ18O
records from many areas of the globe. These similarities suggest that forams can be used to
estimate ice-volume changes and therefore δ18O records from forams are used as a proxy for ice
volume. Similar studies have been conducted on air bubbles extracted on ice cores (e.g., Petit et
39
al. 1999); see Figures 20 and 21). However, some of the best publicized data from ice cores are
the temperature reconstructions derived from a hydrogen isotope (2H -- referred to as deuterium)
that is locked in the ice (Waelbroeck et al. 1995; Masson-Delmotte et al. 2005). Equations that
convert 2H values to temperature values were developed in the 1980s and since then 2H isotopes
have been used to estimate global temperature variation reflected in ice cores (e.g. Lorius et al.
1985 and Waelbroeck et al. 1995).
Figure 20. Vostok Antarctica Ice Coring Station (from NOAA 2009).
Figure 21. Ice Cores in Refrigeration (from NOAA 2009).
40
In addition to reconstructions of temperature using isotopes derived from ice cores,
reconstructions of variation in atmospheric chemistry has become increasingly important. Over
the past 20 years, CO2 and CH4 and extracted from ice cores have been used to reconstruct
changes in atmospheric CO2 during glacial and interglacial periods (Petit et al. 1999). More CO2
and CH4 are present in the atmosphere during interglacial periods because they are linked with
organic matter (Figure 23); during glacial periods ice covers large areas of the northern
hemisphere reducing the amount of area available for colonization by different plants, grasses
and trees.
Variations in CO2 and CH4 have been reconstructed as far back as 160,000 and 414,000 years,
respectively from air bubbles extracted from the Vostok ice core in Antarctica (see Barnola et al.
1987 and Petit et al. 2001). Variations in the CO2 and CH4 recovered from the core are examined
relative to reconstructions of past temperature, sea level, and global ice cover as determined by
other proxy data, to develop an understanding of environmental conditions that existed when
CO2 and CH4 values were different than present (Bradley 1985; Jansen 2007). These
reconstructions are in turn examined relative to variation in earth’s orbital parameters to identify
the correlation between climate change driven by celestial mechanics and the amount of CO2 and
CH4 present in the atmosphere (Randall et al. 2007). These reconstructions indicate that CO2
values ranged from 180 to 297 ppmv over the past 160,000 years, and CH4 values ranged from
319 to 773 ppbv over the past 400,000 years (Petit et al. 2001).
The stomatal density of fossil plants can also be used to estimate past atmospheric CO2 (Reid et
al. 2000). Botanists have demonstrated that under higher levels of CO2 plants become more
efficient and produce fewer stomates; under lower CO2 concentrations they produce more
stomates in order extract adequate CO2 from the atmosphere for conversion into carbohydrates
(Reid et al. 2000). This has been demonstrated by modeling (Roth-Nebelsick et al. 2006) as well
as growing plants in greenhouses with enhanced CO2. Given the results of these studies,
paleontologists speculate that stomatal density in fossil leaves is an indicator of CO2
concentration in the atmosphere.
41
Figure 22. Reconstructions of CO2 (160,000 years to present) and CH4 (400,000 years to present) from Vostok Ice Core, Antarctica (data derived from NOAA). Proxy Data Limitations There are several limitations associated with using proxy data to reconstruct past climate. One
limitation is the assumption that plants and animals living in at different times in the past were
constrained by the same temperature and precipitation as they are today. The greatest limitations
42
of proxy data are errors associated with dating and the inability to reconstruct high frequency
climate variation beyond the length of tree-ring records with any degree of confidence. Below,
limitations of the primary forms of proxy data used to reconstruct climate are discussed.
Limitations of Tree-Rings and Macrobotanical Data
Although higher resolution climate reconstructions can be obtained by analyzing tree-rings and
macro-botanical materials than isotopes these data sets also have limitations. Trees, plants and
grasses take time to respond to changes in environmental conditions; species may die off
relatively quickly in a given area due to climate change, but it generally takes much longer for a
new species to become established in a given area due to climate change (Van Devender et al.
1987). Furthermore:
(t)he first appearance of a plant in a packrat-midden sequence can indicate a climatic
change, but the timing is also subject to the different dispersal capabilities and
migrational distances for individual species. Additionally, although dispersal along an
elevational gradient after a climatic change could be rapid, dispersal along latitudinal
gradients may lag because of differential migration rates. In either case, immigrating
plants may be delayed due to competition if plants with similar ecological adaptation
occupy an area first (Van Devender et al. 1987:325).
Additionally, Van Devender et al. (1987:325) noted that modern analogues of plant assemblages
associated with an ecosystem or ecotone usually differ from paleo-assemblages in some
significant aspect. In particular, plant assemblages were inherently different during glacial
periods from those of today. Similarly, environmental lapse rates for temperature were likely
different in the past than they are today (6.45o C for every 1000 m or 3.56 o F for every 1000 ft)
because the baseline conditions were different. Correspondingly it is somewhat tenuous to apply
modern lapse rates to reconstructions of past environments along an elevational transect.
Limitations of Isotopes: Ice Cores and Foraminifera
Understanding how air bubbles form in ice cores is critical to understanding the limits of using
isotopes trapped in the ice to reconstruct past temperature, precipitation and amounts of trace
gases in the atmosphere. A common misconception is that CO2 recovered from air bubbles
trapped in Arctic and Antarctic ice sheets reflects an annual ‘snap shot’ of these trace gases at a
specific time in earth’s history. In reality, air bubbles do not form at the surface of a glacier, but
rather become trapped at the firn-ice transition about 90 m below a glacier’s surface (Barnola et
al. 1991), and this process can take 100 to 3,000 years depending on climate conditions
(Schwander and Stauffer 1984). During this period, air moves in the ice (horizontally and
43
vertically) and therefore an air bubble that finally becomes trapped in the ice reflects the
atmosphere spanning several decades to several thousands of years, not a single year. As such,
levels of CO2 determined to reflect atmospheric conditions 400,000 years ago, or even 1,000
years ago, based on air bubbles trapped in an ice core reflects average atmospheric conditions
over a period of time—annual and decadal maximum and minim values are not captured.
In addition to the averaging inherent in the sample, before a date (gas age) can be determined for
air bubbles from a band of ice, the snow accumulation rates and regional temperature must be
reconstructed for the period of glacier formation and this information is used to estimate the age
of the ice for different depths using a semi-empirical model. Barnola et al. (1991) developed a
mathematical model to estimate the age of air bubbles by calculating the rate of ice formation
relative to the formation of air bubbles under different climatic conditions. These age
determinations have considerable margins of error associated with them because they are
estimates based on other proxy data (δ18O and 2H isotopes). Additionally, periods of glacial melt
can affect the reliability of ice age determinations; deformation of the ice from the compressive
pressure of the overlying glacier and tensile stress associated with movement of the glacier also
affects the reliability of dates assigned to portions of ice cores (Schwander and Stauffer 1984;
Barnola et al. 1991; Charles et al. 1994; Blunier and Schwander 2000; Bender et al. 2006;
Loulergue et al. 2007). Scientists using Barnola et als. (1991) model determined that air bubbles
in the Vostok ice core, from east Antarctica, were approximately 2000 to 6750 years younger
than the surrounding ice (Petit et al. 1999); the difference is greatest during glacial periods.
Figure 24 illustrates three different temperature reconstructions developed for Vostok using
versions of Barnola et als. model (Lorius et al. 1985; Jouzel et al. 1987 and Jouzel et al. 1993;
Sowers et al. 1993). These reconstructions, derived from the same ice cores, have an
approximately 6,000 year range in when the Eemian interglacial period began and approximately
a 1,350 year range on the timing of the onset of the Holocene (see Figure 23).
Given the lag time that it takes for air bubbles to become trapped in ice (100 – 3,000 years),
dissolution of air through the ice, mixing of water and air in the ice during melt/thaw cycles, and
errors associated with dating the air trapped in ice (2,000 to 6,000 years), scientists need to be
careful to avoid making statements that these reconstructions are directly comparable to present
day values of CO2 and CH4 determined from air sampled by high precession instruments that
take hourly readings at locations all over the world (Earth System Research Laboratory, NOAA
2009d). Conceivably, high frequency variation in atmospheric CO2 and CH4 occurred in the past
but can not be identified in proxy data because of the physical processes of air bubble formation
in ice and the errors discussed above. Additionally, samples extracted from cores are generally
taken in increments of one meter or more; these physical gaps mean that ice is being sampled for
44
atmospheric analysis in roughly 2,000 year increments, precluding identification of high
frequency variation in trace gases in the atmosphere.
Similar to limitations of ice core studies, planktonic (shallow water) and benthic (deep water)
foraminifera also have limitations. For example, foraminifera recovered from deep sea sediment
cores may have died higher in the water column, drifted to the sea floor, been transported along
the sea floor by turbidity and finally deposited only to later be disturbed by bioturbation caused
by burrowing sea life, earthquakes, or deep sea landslides (Mix and Ruddiman 1984; Mix 1987).
As such, the date of deposition of foraminifera recovered from a sediment core may not reflect
the year the animal died or the environment in which it lived. Additionally, studies of the
isotopic composition (δ 13C and δ18O) of shells from living foraminifera indicate that the δ 13C
signatures of most foraminifera reflects the microhabitat in which they lived, rather than the
dissolved inorganic carbon in the bottom-water where they are recovered (Fontanier et al
2008:39). Climate reconstructions derived from foraminifera must, therefore, take into
consideration the microhabitat of the organism when it lived rather than attributing these
conditions to the sediments where the organism was recovered. In addition to these problems,
dating segments of deep sea cores that exceed the threshold for carbon dating (40,000 years)
requires the use of Uranium/Thorium (U/Th) dating methods which has an error of
approximately 3,000 years (Henderson et al. 2001). In summary, the reliability of climate
reconstructions using foraminfera is compromised by the uncertainty associated with the
depositional environment versus the microhabitat in which the organism lived as well as dating
constraints.
Below, reconstructions of past climates are reviewed relative to the dispersal of human
populations across the globe. This section is important for placing current global warming within
the context of long-term climate cycles that the earth has experienced for billions of years, and
humans and their ancestors have faced for over one hundred thousand years.
45
Figure 23. Three Different Temperature Reconstructions using the same Vostok Ice Cores, Antarctica: note differences in peak dates (data derived from NOAA).
46
Archaeology, History and Climate Change Around 135,000 years ago, earth moved from a glacial period into the Eemian interglacial period
which was approximately 4oC warmer than the present interglacial. Sea level was nearly 6 m (~
20 ft) higher than it is today and tropical forests grew as far north as Greenland. This interglacial
lasted approximately 20,000 years, with earth shifting back into a glacial period around 115,000
years ago. During this period temperatures were up to 8oC colder than present in high latitudes
and ice sheets covered virtually all of Canada, and northern regions of Russia, China and Europe.
Like all ice ages, this last ice age was punctuated with periods of slightly warmer conditions that
spanned centuries to millennia, but conditions were not warm enough to cause ice sheets to melt.
The last ice age lasted approximately 100,000 years, with earth moving into the current
interglacial period (the Holocene) about 15,000 years ago (Bradley 1985).
During this period of extreme climatic variation, our ancestors adapted to the punctuated cold
and warm cycles by moving to areas where the fauna and flora were abundant enough to sustain
them. Within the last 40,000 years, modern humans evolved and migrated to every continent on
earth (Morlan 1980; Bonnichsen et al. 1985; Bonnichsen et al. 1987; Bryan 1986; Allen et al.
1995; Bednarik 2000). Archaeologists can reconstruct the movement of past populations across
the landscape by excavating the remains of their camp sites, food processing sites and even areas
where they gathered raw materials to make tools (Bonnichsen et al. 1985; Bonnichsen et al.
1987; Douglas 1990; Bonnichsen et al. 1992; Madsen et al. 2007).
At the end of the last ice age, continental ice sheets and alpine glaciers retreated, opening the
landscape for varieties of grasses, shrubs and trees to become established. As new life took hold
in areas formerly covered by ice, animals and humans could move into these areas. As the ice of
glaciers estimated to be nearly one mile-thick melted (Hughes 1987), sea level rose by hundreds
of feet and people formerly living near the sea moved onto higher. Estuaries and lagoons became
established in many areas that were formerly river beds draining to the sea, providing habitat for
fish, shell fish, birds and plants that could be used for food, clothing, as well as the creation of
other items, such as baskets. The archeological record is replete with prehistoric sites now
buried under hundreds of feet of water and sediment deposited from glacial melt and run-off
from rivers. Since the end of the last ice age earth’s topography has continued to change in
response to the retreat of continental ice sheets. The immense weight of continental ice sheets
compressed earth’s crust and it continues to rebound today; this process has resulted in some
coastal areas that were formerly underwater to rise above sea level (Gutenberg 1941; Farrand
1962; Brevick 1994; Peltier 1944, 1996, 2001). As they were exposed, these areas became open
47
to use by people for habitation and procurement of resources. Throughout human evolution
people have adapted to climate change either by moving into habitable areas or by modifying
inhospitable environments so they would sustain human populations.
Economics of Greenhouse Gas Policies
The IPCC technical reports (Forster et al. 2007; Jansen et al. 2007; Meehl et al. 2007; Randall et
al. 2007), and the summaries written for policymakers (Barker et al. 2007; IPCC 2007a and
2007b) have engendered widespread concern that anthropogenic GHG emissions must be
reduced to below 1990 levels to curb global warming. In response, governments worldwide are
rapidly developing policies to reduce anthropogenic GHG emissions through tax strategies and
by offering incentives for industry and business to adopt cleaner technologies. In a summary
report for the IPCC, Barker et al. (2007) identified means to raise some of the funds necessary to
develop new technologies required to reduce anthropogenic GHG emissions including
establishing:
regulations and standards, taxes and charges, tradable permits, voluntary agreements,
phasing out subsidies and providing financial incentives, research and development and
information instruments. Other policies, such as those affecting trade, foreign direct
investments and social development goals can also affect GHG emissions. In general,
climate change policies, if integrated with other government policies, can contribute to
sustainable development in both developed and developing countries (Barker et al. 2007:
87).
The cost of implementing these types of mitigation measures is calculated on the basis of every
U.S. dollar spent to reduce or eliminate one ton of CO2 equivalent GHG emissions ($US/t CO2-
eq) (Barker et al. 2007). Economists ran several models to determine the cost of reducing CO2-
eq under the different IPCC scenarios studied by the technical analysts (e.g. Forester et al 2007;
Randall et al. 2007). Each combination is referred to in their report as a diversified portfolio
(Barker et al. 2007), and has costs associated with providing incentives for industry and the
public to adopt new technology. An example of potential costs associated with reducing CO2-eq
to 550 ppm under one socio-economic scenario (referred to as Category III stabilization) is
associated with energy sector infrastructure, which “alone is projected to require at least US$29
trillion investment to 2030” and furthermore “the options for (CO2-eq) stabilization will be
heavily constrained by the nature and carbon intensity of the investment” (IPCC 2007a:80).
Other scenarios indicate the costs to change energy infrastructure could be substantially less, but
the ultimate cost is uncertain because of the number of environmental, economic, political and
48
social variables at play. Over time, it is anticipated that investments in mitigation measures
would pay off with the adoption of more efficient technologies.
Global warming scenarios that identify anthropogenic GHG emissions and land use practices as
primary forcing mechanisms indicate that reduced GHG emissions would result in a cessation of
global warming after the atmosphere-ocean circulation system achieved equilibrium. The IPCC
(2007a) ultimately determined that an integrated approach to reducing air pollutants would be the
most cost effective for participating countries. The IPCC noted that “addressing climate change
and air pollution simultaneously through a single set of measures and policies offers potentially
large reductions in the cost of air-pollution control” (2007a:81). In other words, regulations to
modify technology used by large industry should compliment regulations to modify vehicle
emissions.
If controlling anthropogenic GHG emissions and land use practices stopped global warming, the
billions of dollars spent to develop and adopt more efficient technology would be worthwhile.
Attempting to stop global warming by developing and adopting more efficient technology is
admirable, and no doubt will be beneficial to human health and earth’s environment. However,
too little is known about the natural forcing mechanisms that drive climate change to equivocally
state that controlling anthropogenic GHG emissions and reducing CO2 to pre-1990 levels will
have a marked effect on global warming.
Discussion
The IPCC technical reports summarize the current state of knowledge and make best estimates of
what future climate will be like under different anthropogenic GHG emission scenarios.
However, the scientists contributing to the technical reports, clearly state that the current state of
understanding of long-term climate dynamics is incomplete, and can not be adequately modeled
for multiple reasons (Forster et al. 2007; Jansen et al. 2007; Meehl et al. 2007; Randall et al.
2007). Limitations of these investigations are summarized in Tables 3, 4 and 5: the statements in
these tables are direct quotes from the technical reports.
Foremost, the scientific community has focused much of its research and resources on studying
climate change in high latitudes and limited research has been performed in tropical regions.
Leading climate scientists have stated that because of the heat potential of water vapor, it is
critical that we develop a better understanding of fluxes in water vapor in the tropics to truly
grasp what is driving current global warming (e.g. Tim Patterson [see 2005). Further, the IPCC
scientists (Forster et al. 2007) clearly state that water vapor is not adequately addressed in their
models, noting that:
49
Some effects are not quantified, either because they do not have enough evidence or
because their quantification lacks consensus. These include certain mechanisms
associated with land use, stratospheric water vapour and cosmic rays (Forster et al.
2007:200).
and
Deficiencies remain in the simulation of tropical precipitation, the El Niño-Southern
Oscillation and the Madden-Julian Oscillation (an observed variation in tropical winds
and rainfall with a time scale of 30 to 90 days). The ultimate source of most such errors is
that many important small-scale processes cannot be represented explicitly in models,
and so must be included in approximate form as they interact with larger-scale features.
This is partly due to limitations in computing power, but also results from limitations in
scientific understanding or in the availability of detailed observations of some physical
processes (Randall et al. 2007:601).
The scientists reporting for the IPCC note that additional research on water vapor (Forster et al.
2007) and on atmospheric and oceanic circulation in the tropics and Antarctica is needed before
we can understand natural forcing mechanisms driving global warming (Jansen et al. 2007;
Randall et al. 2007). These scientists note that there is a lack of observational data for them to
work with in developing their models, and/or in reconstructing past climate variation at different
regional and temporal scales. If the scientists reporting for the IPCC note that additional research
is needed to understand natural forcing mechanisms of climate change (Forster et al. 2007;
Jansen et al. 2007), and that more computer time is required to adequately model long-term
climate change at a global scale (Randall et al. 2007), why have the IPCC and policymakers
stated that anthropogenic GHG emissions are the primary cause of current global warming?
Punctuated Equilibrium and the Threshold Effect
The author of this paper argues that too little is known about past climate conditions that existed
immediately before the onset of previous ice ages to dismiss the possibility that natural
mechanism are driving the current global warming, and humans are simply accentuating those
conditions. Until scientists have a better understanding of the natural processes affecting climate
change, beyond the 25% explained by orbital forcing and the miniscule percent explained by
volcanism, we can not reliably state that humans are responsible for 75% of the climate change
observed in the past few centuries. The lack of temporal and spatial resolution associated with
reconstructions of past environmental and climatic conditions, combined with our inability to
precisely date the timing, magnitude and amplitude of past climate change, severely minimizes
50
the significance of the IPCC’s statement that recent climate change exceeds the rate and
magnitude of any climate variation that occurred within the past 600,000 years—the resolution
of proxy data that extend climate reconstructions beyond the length of tree-ring records is
inadequate to make such comparisons.
High resolution climate reconstructions derived from tree-ring data (e.g. Graumlich 1993;
Cleaveland et al. 2003; Woodhouse 2003; Pielke et al. 2005) indicate that high-frequency
climate change has occurred over the past 7,000 years. Perhaps the most widely recognized high
frequency climate events reconstructed from tree-rings and historical documents are the
Medieval Warm Period, spanning ca. AD 900 – 1300 (Keigwin 1996; Bradley et al. 2003;
Raymond et al. 2003; Jones and Mann 2004) and the Little Ice Age, spanning ca. AD 1400 - 1850
(Lamb 1977, Grove 1990; Fagan 2001). These events are best documented in Europe, but
reconstructions of past environments elsewhere in the world suggest they may have been global
phenomena (e.g. Thompson et al. 1986; Douglas 1998; Stone 2004; Araneda et al. 2007),
although the timing and magnitude of the events varied by hemisphere and region (Douglas-
Dalziel 2001).
Current limitations of proxy data preclude reconstructing seasonal, annual, decadal, or even
centennial climate variability extending beyond tree-ring records. Given the cyclic nature of
climate, it is very likely that high frequency fluctuations in climate occurred at other times during
the Quaternary period (past 1.8 million years). Further, undoubtedly higher levels of CO2 existed
during warmer cycles than occurred within interglacial periods due to the expansion of
vegetation, but maximum values of CO2 are lost in reconstructions derived from proxy data.
Regardless of high-frequency variations in CO2 values that can not be identified in the proxy
record, it is more critical to understand the atmospheric and oceanic dynamics that occurred at
the end of the last interglacial in order to identify natural forcing mechanisms that may be
driving recent global warming. Based on celestial mechanics, the current interglacial should be
ending and earth should be entering another glacial epoch (Imbrie and Imbrie 1980; Ruddiman et
al. 2005; Douglas 2007a and 2007b; Stuckless and Levitch 2007). Although earth’s orbital
parameters were different at the end of the last interglacial cycle than they are today, similar
climate dynamics reflecting earth moving from an interglacial period and into a glacial period
may be expected. It is important to reiterate that celestial mechanics only explain approximately
25% of climate change (Imbrie and Imbrie 1980), and therefore other natural forcing
mechanisms must explain how the earth shifts between glacial and interglacial cycles.
The ocean is earth’s largest body of stored heat energy followed by water vapor in the
atmosphere. As such, changes in the dynamics of these systems likely drives shifts between
51
glacial and interglacial periods. During interglacial periods, considerable heat and CO2 are
stored in the ocean. Low-frequency climate change associated with celestial mechanics drives
the atmospheric-ocean circulation system and these systems are in relative equilibrium for
several thousand years until they reach a temperature or salinity threshold that forces rapid
change in the systems. Recent global warming may reflect water vapor and CO2 that is stored in
the ocean into the atmosphere through evaporation in low latitudes—this process would enhance
the greenhouse effect and result in rapid global warming. Increased water vapor in tropical
regions would also result in increased precipitation in low latitudes. Higher levels of
precipitation and runoff would result in more fresh water being fed into the Gulf Stream, which
would carry higher volumes of relatively fresh water into the North Atlantic.
Several climate models indicate that an influx of fresh water into the North Atlantic could slow
and/or stop the formation of the NADW current and the MOC, potentially causing the onset of a
glacial period (Rahmstorf et al. 2005). Although some scholars speculate that anthropogenic
GHG emissions are keeping earth from entering an ice age, the author would argue that there is
insufficient understanding of the natural dynamics associated with shifts between interglacial and
glacial periods to reliably make a statement that anthropogenic GHG emissions can stop the
onset of an ice age. Until a comprehensive understanding of the natural forcing mechanisms that
drove past glacial and interglacial cycles is obtained we can not truly understand human impacts
on these systems.
Below, the author recommends areas where additional research might enhance scientific
understanding of climate conditions that occurred near the end of the last interglacial, and
facilitate identification of natural forcing mechanisms driving current global warming.
Understanding the natural forcing mechanisms underlying high frequency climate change that
occurred at the end of the last interglacial period is the only way scientists will be able to
determine the degree to which anthropogenic effects are driving current global warming with a
high level of statistical certainty.
Research Suggestions
Paleoenvironmental Reconstructions Ice cores: Additional studies on the diffusion of air in ice under different temperatures and
pressures might contribute understanding to how much atmospheric CO2 varied (minimums and
maximums) at different times during the Quaternary period.
Deep-sea sediment cores from the tropics and subtropics: We need to develop a more
comprehensive understanding of low- and high-frequency changes in oceanic circulation (surface
52
and deep currents) near the equator, so we can better understand changes in the distribution of
heat energy, and diffusion of CO2 at the ocean-atmosphere interface.
Sediment cores from relict lakes in tropical and subtropical regions of Africa, Asia and South
America: These studies may shed light on changes in the location and intensity of the ITCZ
through time—a system which has considerable impact on the hydrologic cycle.
Deep-sea sediment cores Antarctica: Scientists have little understanding of the dynamic
coupling associated with ocean currents and sea ice in Antarctica—additional marine studies
may shed light on these systems and how they have changed through time.
Hydrothermal vents and submarine volcanoes: These systems cover thousands of miles of our
ocean floors and are extremely dynamic. Understanding the amount of thermal energy and gases
emitted from these systems would contribute significant understanding to changes in earth’s heat
balance, as well as conceivably fluctuations in ocean acidity.
Modeling Climate models are essential for simulating earth’s complex physical dynamics and human
impacts on natural climate systems. It is a shame that the climate scientists tasked with obtaining
an understanding of these dynamics and systems do not have adequate funding to run the models
required to study natural forcing mechanisms at a global scale. As with establishing a better
baseline of proxy data, more funding is required to pay for longer run-times of more complex
AOGCMs, as well as to pay for verifying these models.
Conclusions
Governments have dedicated hundreds of billions of dollars to developing and adopting more
energy efficient technologies in a ‘panic’ to stop global warming. The author of this paper
recommends that a percentage of this money be dedicated to unbiased scientific research to
develop a solid baseline identifying natural climate forcing mechanisms so that future
generations can truly understand how human behavior affects long-term climate cycles. The
IPCC’s mandate to study human-induced impacts on global warming precludes IPCC scientists
from studying the natural forcing mechanisms that underlie the anthropogenic signature of
climate change to the degree required to understand the causes of recent global warming. As
highlighted in Tables 3, 4 and 5, the scientists reporting to the IPCC note insufficient research,
poor understanding of natural forcing mechanisms (Forster et al. 2007; Jansen et al. 2007), and
inadequate funding to run high resolution AOGCM models for the period of time required to
identify natural dynamics driving climate change (Randall et al. 2007); these scientists focused
53
on what they were funded to focus on: Human-induced climate change. In contrast, large
industry often funds research on natural cycles of climate variability, but this research has
typically been focused on climate change that has occurred within the past few thousand years.
The results of these studies are often used to counter the results of the IPCC. For examples of
organizations Greenpeace identified as being funded by Exxon to develop counter arguments to
the global warming debate:
http://www.exxonsecrets.org/html/list organizations.php
Because these scientists accepted funding from large industry, their arguments are often
dismissed as biased (Gore 2006; Littlemoore 2006; Michaels 2009, Reinhard 2008). However,
this argument could equally be applied to the IPCC technical reports which were funded to focus
on human-induced climate change.
If earth experiences global warming of the magnitude that occurred during the last interglacial
period, sea level will rise by 5 to 6 m and atmospheric and oceanic circulation will change
significantly. The rise in sea level and changes in circulation will flood thousands of miles of
coast line and result in more intensive storms in some regions and severe drought in others. In
addition to loss of life and property, the composition and distribution of terrestrial and marine
flora and fauna that people rely upon for subsistence will change dramatically. Lands that are
currently arable could become desolate wastelands due to water shortages and extreme
temperatures. Cities and villages located on the edge of dune-fields could become buried in sand
as deserts expand into formerly vegetated landscapes. Social and economic stresses will
skyrocket as humanity attempts to adapt to extreme changes in their environment with limited
financial resources.
If controlling anthropogenic GHG emissions could stop or stem these conditions, the hundreds of
billions of dollars dedicated to develop and adopt green technologies will be well spent. If,
however, natural forcing mechanisms are the primary cause of current global warming and
anthropogenic effects are only accentuating these mechanisms, billions of dollars that could have
been allocated to: moving coastal populations to higher ground, helping the fishing industry
adapt to changes in the composition and distribution of marine organisms used for subsistence,
developing desalination plants to reduce the effects of water shortages, and establishing an
infrastructure that can support earth’s growing population on reduced/stressed land area, then
perhaps a portion of this money would be better spent planning to adapt to climate change that is
imminent. With so much at risk, it is time to lay down the gloves and identify a strategy for
studying the interplay of natural and anthropogenic climate forcing so we can better plan for the
future using the global community’s limited financial resources.
54
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Appendix 1. IPCC Energy Moisture Balance Models and their Parameters
Name Atmosphere Ocean Sea Ice Coupling Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E1: BERN2.5CC E1: BERN2.5CC (Plattner et al., 2001;Joos et al., 2001)
EMBM, 1-D (ϕ), NCL,7.5° x 15° (Schmittner and Stocker, 1999)
FG with parametrized zonal pressure gradient,
2-D (ϕ, z), 3 basins, RL,
0-LT, 2-LIT (Wright and Stocker, 1993)
PM, NH, NW (Stocker et al., 1992; Schmittner and Stocker, 1999)
NST, NSM (Schmittner and Stocker, 1999)
BO (Marchal et al., 1998),BT (Sitch et al., 2003;Gerber et al., 2003),BV (Sitch et al., 2003;Gerber et al., 2003)
Energy moisture
balance model;zonally and vertically averaged;
ISO, MESO, 7.5°x15° , 14L(Wright and Stocker, 1992)
0-layer thermodynamic scheme two-level ice thickness distribution (level ice and leads).
Prescribed momentum flux no heat flux adjustmentno fresh water flux adjustment
No explicit computation of soil temperature no moisture storage in soil
Model of oceanic carbon dynamics model of terrestrial carbon dynamics;dynamical vegetation model.
Non-interacive
cloudiness Frictional geostrophic model with parameterized zonal pressure gradient, 2 dimensional, zonally averaged three basins; rigid lid isopycnal diffusion; parametrization of the effect
7.5 x 15 degree grid
7.5 x 15 degree grid
68
Appendix 1. IPCC Energy Moisture Balance Models and their Parameters (Continued)
Name Atmosphere Ocean Sea Ice Coupling Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E2: C-GOLDSTEIN E2: C-GOLDSTEIN (Edwards and Marsh, 2005)
EMBM, 2-D(ϕ, λ), NCL, 5° x 10° (Edwards and Marsh, 2005)
FG, 3-D, RL, ISO, MESO, 5° x 10°, L8 (Edwards and Marsh, 2005)
0-LT, DOC, 2-LIT (Edwards and Marsh, 2005)
GM, NH, RW (Edwards and Marsh, 2005)
NST, NSM, RIV (Edwards and Marsh, 2005)
Energy moisture
balance model; vertically averaged; non-interactive cloudiness; 5 x 10 degree grid
Frictional geostrophic model three dimensional rigid lid isopycnal diffusion; parametrization of the effect 5 x 10 degree grid 8 levels
0-layer thermodynamic scheme drift with ocean currents two-level ice thickness distribution (level ice and leads).
Global momentum flux adjustment no heat flux adjustment regional fresh water flux adjustment
No explicit computation of soil temperature no moisture storage in soil river routing scheme
Model E3:CLIMBER-2 E3: CLIMBER-2 (Petoukhov et al.,2000)
SD, 3-D, CRAD, ICL, 10° x 51°, L10 (Petoukhov et al., 2000)
FG with parametrized zonal pressure gradient,
2-D (ϕ, z), 3 basins, RL, 2.5°, L21 (Wright and
0-LT, DOC, 2-LIT (Petoukhov et al., 2000)
NM, NH, NW (Petoukhov et al., 2000)
1-LST, CSM, RIV (Petoukhov et al., 2000)
BO (Brovkin et al., 2002), BT (Brovkin et al., 2002), BV (Brovkin et al., 2002)
TM, 3-D, 0.75° x 1.5°, L20* (Calov et al., 2005)
Statistical
dynamical model; comprehensive radiation scheme 3 dimensional interactive cloudiness 10 levels 10 x 51 degree grid
Frictional geo-strophic model with parameterized zonal pressure gradient, 2 dimensional zonally averaged, 3 basins; rigid lid 2.5 degree grid, 21 L
0-layer thermodynamic scheme drift with ocean currents two-level ice thickness distribution (level ice and leads).
No momentum flux adjustment no heat flux adjustment no fresh water flux adjustment
1-layer soil temperature scheme complex model for soil moisture river routing scheme
Model of oceanic carbon dynamics model of terrestrial carbon dynamics; dynamical vegetation model.
69
Appendix 1. IPCC Energy Moisture Balance Models and their Parameters (Continued)
Name Atmosphere Ocean Sea Ice Coupling Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E4: CLIMBER-3a E4: CLIMBER-3a (Montoya et al., 2005)
SD, 3-D, CRAD, ICL, 7.5° x 22.5°, L10 (Petoukhov et al., 2000)
PE, 3-D, FS, ISO, MESO, TCS, DC*, 3.75° x 3.75°, L24 (Montoya et al., 2005)
2-LT, R, 2-LIT (Fichefet and Morales Maqueda, 1997)
AM, NH, RW (Montoya et al., 2005)
1-LST, CSM, RIV (Petoukhov et al., 2000)
BO* (Six and Maier-Reimer, 1996), BT* (Brovkin et al., 2002), BV* (Brovkin et al., 2002)
Statistical
dynamical model; comprehensive radiation scheme 3 dimensional interactive cloudiness
Primitive equation model 3-dimensional; free surface isopycnal diffusion; parametrization of the effect complex turbulence closure scheme parametrization of density-driven down-sloping currents
2-layer thermodynamic scheme viscous-plastic or elastic-viscous-plastic rheology two-level ice thickness distribution (level ice and leads).
Momentum fl ux anomalies relative to the control run are computed and added to climatological data no heat flux adjustment regional fresh water flux adjustment
1-layer soil temperature scheme complex model for soil moisture river routing scheme
Model of oceanic carbon dynamics model of terrestrial carbon dynamics;dynamical vegetation model.
10 levels 7.5 x 22.5 degree grid
24 levels 3.75 x 3.75 degree grid
70
Appendix 1. IPCC Energy Moisture Balance Models and their Parameters (Continued) Name Atmosphere Ocean Sea Ice Coupling
Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E5: LOVECLIM E5: LOVECLIM (Driesschaert, 2005)
QG, 3-D, LRAD, NCL, T21 (5.6° x 5.6°), L3, (Opsteegh et al.,1998)
PE, 3-D, FS, ISO, MESO, TCS, DC, 3° x 3°, L30, (Goosse and Fichefet, 1999)
3-LT, R, 2- LIT (Fichefet and Morales Maqueda, 1997)
NM, NH, RW (Driesschaert., 2005)
1-LST, BSM, RIV (Opsteegh et al., 1998)
BO (Mouchet and François, 1996), BT (Brovkin et al., 2002), BV (Brovkin et al., 2002)
TM, 3-D, 10 km x 10 km, L30 (Huybrechts, 2002)
Quasi-geostrophic model three dimensional linearized radiaiton scheme non-interactive cloudiness
Primitive equation model 3-dimensional; free surface isopycnal diffusion; parametrization of the effect complex turbulence closure scheme parametrization of density-driven down-sloping currents
3-layer thermodynamic scheme viscous-plastic or elastic-viscous-plastic rheology two-level ice thickness distribution (level ice and leads).
No momentum flux adjustment no heat flux adjustment regional fresh water flux adjustment
1-layer soil temperature scheme bucket model for soil moisture river routing scheme
Model of oceanic carbon dynamics model of terrestrial carbon dynamics;dynamical vegetation model.
71
Appendix 1. IPCC Energy Moisture Balance Models and their Parameters (Continued)
Name Atmosphere Ocean Sea Ice Coupling Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E6: MIT-IGSM2.3
E6: MIT-IGSM2.3 (Sokolov et al., 2005)
T21(?) 3 vertical levels 5.6 x 5.6 degree grid SD,
2-D (ϕ, z), CRAD, ICL, 4°, L11 (Sokolov and Stone, 1998), CHEM* (Mayer et al.,2000)
3 x 3 degree grid 30 levels PE, 3-D, FS, ISO, MESO, 4° x 4°, L15 (Marshall et al., 1997)
3-LT, 2-LIT (Winton, 2000)
AM, GH, GW (Sokolov et al., 2005)
BO (Parekh et al., 2005), BT (Felzer et al., 2005), BV* (Felzer et al., 2005)
Statistical
dynamical model; Zonally averaged; comprehensive radiation scheme interactive cloudiness 4 degree grid 11 veritcal levels
Primitive equation model 3-dimensional; free surface isopycnal diffusion; parametrization of the effect 4 x 4 degree grid 15 levels
3-layer thermodynamic scheme two-level ice thickness distribution (level ice and leads).
Momentum fl ux anomalies relative to the control run are computed and added to climatological data global heat flux adjustment global freshwater adjustment
10-layer soil temperature scheme complex model for soil moisture
Model of oceanic carbon dynamics model of terrestrial carbon dynamics; dynamical vegetation model.
72
Appendix 1. IPCC Energy Moisture Balance Models and their Parameters (Continued)
Name Atmosphere Ocean Sea Ice Coupling Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E7: MOBIDIC E7: MOBIDIC (Crucifi x et al., 2002)
QG, 2-D (ϕ, z), CRAD, NCL, 5°, L2 (Gallée et al., 1991)
PE with parametrized zonal pressure gradient,
2-D (ϕ, z), 3 basins, RL, DC, 5°, L15 (Hovine and Fichefet, 1994)
0-LT, PD, 2-LIT (Crucifi x et al., 2002)
NM, NH, NW (Crucifi x et al., 2002)
1-LST, BSM (Gallée et al., 1991)
BO* (Crucifi x, 2005), BT* (Brovkin et al., 2002), BV (Brovkin et al., 2002)
M, 1-D (ϕ), 0.5° (Crucifi x and Berger, 2002)
Quasi-
geostrophic model zonally averaged comprehensive radiation scheme non-interactive cloudiness 2 vertical levels
Primitive equation with parametrized zonal pressure gradient, 2 dimensional zonally averaged; 3 basins; rigid lid parametrization of density-driven down-sloping currents 5 degree grid 15 levels
0-layer thermodynamic scheme prescribed drift two-level ice thickness distribution (level ice and leads).
No momentum flux adjustment no heat flux adjustment no fresh water flux adjustment
1-layer soil temperature scheme bucket model for soil moisture
Model of oceanic carbon dynamics model of terrestrial carbon dynamics; dynamical vegetation model.
73
Appendix 1. IPCC Energy Moisture Balance Models and their Parameters (Continued)
Name Atmosphere Ocean Sea Ice Coupling Flux/Adjustments Land Surface Biosphere Ice Sheets
Model E8: UVIC E8: UVIC (Weaver et al., 2001)
DEMBM, 2-D
(ϕ, λ), NCL, 1.8° x 3.6° (Weaver et al., 2001)
PE, 3-D, RG, ISO, MESO, 1.8° x 3.6° (Weaver et al., 2001)
0-LT, R, 2-LIT (Weaver et al., 2001)
AM, NH, NW (Weaver et al., 2001)
1-LST, CSM, RIV (Meissner et al., 2003)
BO (Weaver et al., 2001), BT (Cox, 2001), BV (Cox, 2001)
M, 2-D (ϕ, λ), 1.8° x 3.6°* (Weaver et al., 2001)
Energy moisture balance model with some dynamics vertically averaged non-interactive cloudiness 1.8 x 3.6 degree grid
0-layer thermodynamic scheme viscous-plastic or elastic-viscous-plastic rheology two-level ice thickness distribution (level ice and leads).
Momentum fl ux anomalies relative to the control run are computed and added to climatological data no heat flux adjustment no fresh water flux adjustment
1-layer soil temperature scheme complex model for soil moisture river routing scheme
Model of oceanic carbon dynamics model of terrestrial carbon dynamics;
Note: a EMBM = energy-moisture balance model; DEMBM = energy-moisture balance model including some dynamics; SD = statistical-dynamical model; QG = quasi-
geostrophic model; 1-D (ϕ) = zonally and vertically averaged; 2-D(ϕ, λ) = vertically averaged; 2-D(ϕ, z) = zonally averaged; 3-D = three-dimensional; LRAD = linearized radiation scheme; CRAD = comprehensive radiation scheme; NCL = non-interactive cloudiness; ICL = interactive cloudiness; CHEM = chemistry module; horizontal and vertical resolutions: the horizontal resolution is expressed either as degrees latitude x longitude or as spectral truncation with a rough translation to degrees latitude x longitude;
the vertical resolution is expressed as ‘Lm’, where m is the number of vertical levels. b FG = frictional geostrophic model; PE = primitive equation model; 2-D (ϕ, z) = zonally averaged; 3-D = three-dimensional; RL = rigid lid; FS = free surface; ISO = isopycnal diffusion; MESO = parametrization of the effect of mesoscale eddies on tracer distribution; TCS = complex turbulence closure scheme; DC = parametrization of density-driven down-sloping currents; horizontal and resolutions: the horizontal resolution is expressed as degrees latitude x longitude; the vertical resolution is expressed as ‘Lm’, where m is the number of vertical levels.c n-LT = n-layer thermodynamic scheme; PD = prescribed drift; DOC = drift with oceanic currents; R = viscous-plastic or elastic-viscous-plastic rheology; 2-LIT = two-level ice thickness distribution (level ice and leads). Notes (continued):d PM = prescribed momentum fl ux; GM = global momentum fl ux adjustment; AM = momentum fl ux anomalies relative to the control run are computed and added to climatological data; NM = no momentum fl ux adjustment; GH = global heat fl ux adjustment; NH = no heat fl ux adjustment; GW = global freshwater fl ux
adjustment; RW = regional freshwater fl ux adjustment; NW = no freshwater fl ux adjustment.e NST = no explicit computation of soil temperature; n-LST = n-
layer soil temperature scheme; NSM = no moisture storage in soil; BSM = bucket model for soil moisture; CSM = complex model for soil
moisture; RIV = river routing scheme.f BO = model of oceanic carbon dynamics; BT = model of terrestrial carbon dynamics; BV = dynamical
vegetation model. g TM = thermomechanical model; M = mechanical model (isothermal); 1-D (ϕ) = vertically averaged with east-west parabolic profi le; 2-
D (ϕ, λ) = vertically averaged; 3-D = three-dimensional; horizontal and vertical resolutions: the horizontal resolution is expressed either as degrees latitude x longitude or kilometres x kilometres; the vertical resolution is expressed as ‘Lm’, where m is the number of vertical levels.