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The Oceanic Sink for Anthropogenic CO2

Christopher L. Sabine,1* Richard A. Feely,1 Nicolas Gruber,2 Robert M. Key,3 Kitack Lee,4 John L. Bullister,1 Rik Wanninkhof,5 C. S. Wong,6 Douglas W. R. Wallace,7 Bronte Tilbrook,8 Frank J. Millero,9 Tsung-Hung Peng,5 Alexander Kozyr,10 Tsueno Ono,11 Aida F. Rios12

1National Oceanic and Atmospheric Administration (NOAA) Pacific Marine Environmental Laboratory, 7600 Sand Point Way NE, Seattle, WA 98115, USA.
2University of California–Los Angeles, Institute of Geophysics and Planetary Physics and Department of Atmospheric and Oceanic Sciences, Los Angeles, CA 90095, USA.
3Princeton University, Program in Atmospheric and Oceanic Science, Forrestal Campus/Sayre Hall, Princeton, NJ 08544, USA.
4Pohang University of Science and Technology, San 31, Nam-gu, Hyoja-dong, Pohang 790-784, South Korea.
5NOAA Atlantic Oceanographic and Meteorological Laboratory, 4301 Rickenbacker Causeway, Miami, FL 33149, USA.
6Institute of Ocean Sciences, Climate Chemistry Laboratory, Post Office Box 6000, Sidney, BC V8L 4B2, Canada.
7Forschungsbereich Marine Biogeochemie, Leibniz Institut für Meereswissenschafte, an der Universität Kiel, (IFM-GEOMAR), Düsternbrooker Weg 20, D-24105 Kiel, Germany.
8Commonwealth Scientific and Industrial Research Organisation (CSIRO) Marine Research and Antarctic Climate and Ecosystem Cooperative Research Center, Hobart, Tasmania 7001, Australia.
9University of Miami, Rosenstiel School of Marine and Atmospheric Science, Division of Marine and Atmospheric Sciences, 4600 Rickenbacker Causeway, Miami, FL 33149, USA.
10Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Mail Stop 6335, Oak Ridge, TN 37831–6335, USA.
11Frontier Research System for Global Change/Institute for Global Change Research, Sumitomo Hamamatsu-cho, Building 4F, 1-18-16 Hamamatsutyo, Minato-ku, 105-0013, Japan.
12Instituto de Investigaciones Marinas, Consejo Superior de Investigationes Cientificas, c/Eduardo Cabello, 6, 36208 Vigo, Spain.

Science, 305(5682), 367–371 (2004)
Copyright ©2004 by The American Association for the Advancement of Science. Further electronic distribution is not allowed.

Abstract

Using inorganic carbon measurements from an international survey effort in the 1990s and a tracer-based separation technique, we estimate a global oceanic anthropogenic carbon dioxide (CO) sink for the period from 1800 to 1994 of 118 ± 19 petagrams of carbon. The oceanic sink accounts for ~48% of the total fossil-fuel and cement-manufacturing emissions, implying that the terrestrial biosphere was a net source of CO to the atmosphere of about 39 ± 28 petagrams of carbon for this period. The current fraction of total anthropogenic CO emissions stored in the ocean appears to be about one-third of the long-term potential.


Since the beginning of the industrial period in the late 18th century, i.e., over the anthropocene [Crutzen and Stoermer, 2000], humankind has emitted large quantities of CO into the atmosphere, mainly as a result of fossil-fuel burning, but also because of land-use practices, e.g., deforestation [Houghton and Hackler, 2002]. Measurements and reconstructions of the atmospheric CO history reveal, however, that less than half of these emissions remain in the atmosphere [Prentice et al., 2001]. The anthropogenic CO that did not accumulate in the atmosphere must have been taken up by the ocean, by the land biosphere, or by a combination of both. The relative roles of the ocean and land biosphere as sinks for anthropogenic CO over the anthropocene are currently not known. Although the anthropogenic CO budget for the past two decades, i.e., the 1980s and 1990s, has been investigated in detail [Prentice et al., 2001], the estimates of the ocean sink have not been based on direct measurements of changes in the oceanic inventory of dissolved inorganic carbon (DIC).

Recognizing the need to constrain the oceanic uptake, transport, and storage of anthropogenic CO for the anthropocene and to provide a baseline for future estimates of oceanic CO uptake, two international ocean research programs, the World Ocean Circulation Experiment (WOCE) and the Joint Global Ocean Flux Study (JGOFS), jointly conducted a comprehensive survey of inorganic carbon distributions in the global ocean in the 1990s [Wallace, 2001]. After completion of the U.S. field program in 1998, a 5-year effort was begun to compile and rigorously quality-control the U.S. and international data sets, including a few pre-WOCE data sets in regions that were data limited [Key et al., in preparation]. The final data set consists of 9618 hydrographic stations collected on 95 cruises, which represents the most accurate and comprehensive view of the global ocean inorganic carbon distribution available [1]. As individual basins were completed, the ocean tracer–based C* method [Gruber et al., 1996] was used to separate the anthropogenic CO component from the measured DIC concentrations [Sabine et al., 1999; Sabine et al., 2002; Lee et al., 2003]. Here we synthesize the individual ocean estimates to provide an ocean data-constrained global estimate of the cumulative oceanic sink for anthropogenic CO for the period from ~1800 to 1994 [2].

Distribution and inventories of anthropogenic CO2 in the ocean. The objectively gridded individual sample estimates were vertically integrated to produce the column inventory map shown in Fig. 1. Because the global survey had limited data coverage in the marginal basins and the Arctic Ocean (north of 65°N), these areas were excluded from the mapped regions. The cumulative oceanic anthropogenic CO sink in 1994, for the ocean region shown in Fig. 1, is 106 ± 17 Pg C. Accounting for the excluded regions, we estimate a global anthropogenic CO sink of 118 ± 19 Pg C. The uncertainty in the total inventory is based on uncertainties in the anthropogenic CO estimates and mapping errors [2].

Figure 1

Fig. 1. Column inventory of anthropogenic CO in the ocean (mol m). High inventories are associated with deep water formation in the North Atlantic and intermediate and mode water formation between 30° and 50°S. Total inventory of shaded regions is 106 ± 17 Pg C.

Figure 1 shows that this anthropogenic CO is not evenly distributed throughout the oceans. The highest vertically integrated concentrations are found in the North Atlantic. As a result, this ocean basin stores 23% of the global oceanic anthropogenic CO, despite covering only 15% of the global ocean area (table S1). By contrast, the Southern Ocean south of 50°S has very low vertically integrated anthropogenic CO concentrations, containing only 9% of the global inventory. More than 40% of the global inventory is found in the region between 50°S and 14°S because of the substantially higher vertically integrated concentrations and the large ocean area in these latitude bands (Fig. 1, table S1). About 60% of the total oceanic anthropogenic CO inventory is stored in the Southern Hemisphere oceans, roughly in proportion to the larger ocean area of this hemisphere.

Figure 2 shows the anthropogenic CO distributions along representative meridional sections in the Atlantic, Pacific, and Indian oceans for the mid-1990s. Because anthropogenic CO invades the ocean by gas exchange across the air-sea interface, the highest concentrations of anthropogenic CO are found in near-surface waters. Away from deep water formation regions, the time scales for mixing of near-surface waters downward into the deep ocean can be centuries, and as of the mid-1990s, the anthropogenic CO concentration in most of the deep ocean remained below the detection limit for the C* technique.

Figure 2

Fig. 2. Representative sections of anthropogenic CO (mol kg) from (A) the Atlantic, (B) Pacific, and Indian (C) oceans. Gray hatched regions and numbers indicate distribution of intermediate water masses (and North Atlantic Deep Water) on the given section and the total inventory of anthropogenic CO (Pg C) within these water masses. The southern water masses in each ocean represent Antarctic Intermediate Water. The northern water masses represent the North Atlantic Deep Water (A), North Pacific Intermediate Water (B), and Red Sea/Persian Gulf Intermediate Water (C). The two bold lines in each panel give the potential density [ = (density – 1) × 1000] contours for the surfaces shown in Fig. 4. Insets show maps of the cruise tracks used. Note that the depth scale for (A) is twice that of the other figures, reflecting the deeper penetration in the North Atlantic.

Variations in surface concentrations are related to the length of time that the waters have been exposed to the atmosphere and to the buffer capacity, or Revelle factor, for seawater [Revelle and Suess, 1957; Takahashi et al., 1993]. This factor describes how the partial pressure of CO in seawater (PCO) changes for a given change in DIC. Its value is proportional to the ratio between DIC and alkalinity, where the latter term describes the oceanic charge balance. Low Revelle factors are generally found in the warm tropical and subtropical waters, and high Revelle factors are found in the cold high latitude waters (Fig. 3). The capacity for ocean waters to take up anthropogenic CO from the atmosphere is inversely proportional to the value of the Revelle factor; hence, the lower the Revelle factor, the higher the oceanic equilibrium concentration of anthropogenic CO for a given atmospheric CO perturbation. The highest anthropogenic CO concentrations (~60 mol kg) are found in the subtropical Atlantic surface waters because of the low Revelle factors in that region. By contrast, the nearsurface waters of the North Pacific have a higher Revelle factor at comparable latitudes and consequently lower anthropogenic CO concentrations primarily because North Pacific alkalinity values are as much as 100 mol kg lower than those in the North Atlantic (Fig. 3).

Figure 3

Fig. 3. Map of the 1994 distribution of Revelle factor, (PCO/DIC)/ (PCO/DIC), averaged for the upper 50 m of the water column. A high Revelle factor indicates that, for a given atmospheric CO perturbation, the oceanic equilibrium concentration of anthropogenic CO will be lower than that for low–Revelle factor waters. The current Revelle factors are about one unit higher than they were in the preindustrial ocean.

About 30% of the anthropogenic CO is found at depths shallower than 200 m and nearly 50% at depths above 400 m. The global average depth of the 5 mol kg contour is ~1000 m. The majority of the anthropogenic CO in the ocean is, therefore, confined to the thermocline, i.e., the region of the upper ocean where temperature changes rapidly with depth. Variations in the penetration depth of anthropogenic CO are determined by how rapidly the anthropogenic CO that has accumulated in the near-surface waters is transported into the ocean interior. This transport occurs primarily along surfaces of constant density called isopycnal surfaces.

The deepest penetrations are associated with convergence zones at temperate latitudes where water that has recently been in contact with the atmosphere can be transported into the ocean interior. The isopycnal surfaces in these regions tend to be thick and inclined, providing a pathway for the movement of anthropogenic CO-laden waters into the ocean interior. Low vertical penetration is generally observed in regions of upwelling, such as the Equatorial Pacific, where intermediate-depth waters, low in anthropogenic CO, are transported toward the surface. The isopycnal layers in the tropical thermocline tend to be shallow and thin, minimizing the movement of anthropogenic CO-laden waters into the ocean interior.

Figure 4A shows the distribution of anthropogenic CO on a relatively shallow isopycnal surface (see depths in Fig. 2) with a potential density () of 26.0. About 20% of the anthropogenic CO is stored in waters with potential densities equal to or less than that of this surface. The highest concentrations are generally found closest to where this density intersects the surface, an area referred to as the outcrop. Concentrations decrease away from these outcrops in the Indian and Pacific oceans, primarily reflecting the aging of these waters, i.e., these waters were exposed to lower atmospheric CO concentrations when they were last in contact with the atmosphere. The Atlantic waters do not show this trend because the 26.0 surface is much shallower and therefore relatively well connected to the ventilated surface waters throughout most of the Atlantic (Figs. 2A and 4A).

Figure 4

Fig. 4. Maps of anthropogenic CO on the (A) 26.0 and (B) 27.3 potential density surfaces. Bold lines at the edge of the colored region indicate areas where the density surface outcrops. The highest values are generally observed closest to the outcrop and decrease toward the equator.

The formation and transport of mode and intermediate waters is the primary mechanism for moving anthropogenic CO to intermediate depths. The spatial distribution of anthropogenic CO in these intermediate waters is illustrated with the 27.3 surface (Fig. 4B), whose mean depth is about 900 m. As with the 26.0 surface, anthropogenic CO concentrations decrease away from the outcrop. On this deeper surface, however, slower ventilation results in stronger gradients and large areas where the anthropogenic CO is below detection level. The Atlantic contains substantially higher anthropogenic CO concentrations on the 27.3 surface than the other basins, due in part to faster ventilation, but also because of the more favorable Revelle factor. Although the formation of intermediate, mode, and deep waters provides the primary mechanism for moving anthropogenic CO into the ocean interior, the magnitude and distribution of the anthropogenic signal can be quite different depending on the nature of the water mass. As examples, some of the dominant intermediate water masses are outlined in Fig. 2 [3].

Antarctic Intermediate Water (AAIW) is formed in the Southern Ocean from upwelled Circumpolar Deep Water in the vicinity of the Subantarctic Front between 45° and 55°S and is then subducted and transported northward at intermediate depths. Immediately north of the AAIW, sub-Antarctic Mode Water (SAMW) forms north of the sub-Antarctic Front and contains a greater component of subtropical water than AAIW and is also subducted into the main thermocline of the ocean interior. While at the surface, these water masses appear to take up large amounts of anthropogenic CO from the atmosphere as a result of both high wind speeds enhancing gas transfer and low initial anthropogenic CO content. These subducted intermediate and mode waters contain high concentrations of anthropogenic CO, which are transported equatorward and downward, as clearly evidenced by the deepening of anthropogenic CO penetration in Fig. 2. This transport plus the large volumetric contribution of the water masses to the Southern Hemisphere thermocline leads to high anthropogenic CO inventories, estimated to exceed 20 Pg C [3].

About 3.2 Pg of anthropogenic carbon is found in the North Pacific Intermediate Water (NPIW). Unlike the AAIW that typically delineates the lower limit of the anthropogenic penetration, a substantial amount of anthropogenic CO can be found deeper than the NPIW at the latitude of the section shown in Fig. 2B. NPIW is not the only intermediate- type water mass formed in the North Pacific, and the complex interplay of different intermediate-type waters in the North Pacific makes it difficult to attribute the anthropogenic signal to any one specific intermediate water mass in this region.

Nearly 3 Pg C can be found in the intermediate waters of the northern Indian Ocean (Fig. 2C). The Indian Ocean differs from the other oceans because of its land-locked northern boundary. Anthropogenic CO in the tropical north Indian Ocean generally penetrates deeper than in the tropical Atlantic and Pacific. This primarily reflects the introduction of relatively young, dense waters that are high in anthropogenic CO from the Red Sea and the Persian Gulf [Sabine et al., 1999; Papaud and Poisson, 1986; Mecking and Warner, 1999]. Excess evaporation in these regions increases the salinity and density of the waters, which sink and carry the anthropogenic CO with them. As these waters flow into the northern Indian Ocean at intermediate depths, they mix and spread equatorward across the northern Indian Ocean.

Globally, only 7% of the total anthropogenic CO is found deeper than 1500 m. The only place where large concentrations of anthropogenic CO penetrate to mid and abyssal depths is the North Atlantic, as a result of the formation and downward spreading of Labrador Sea Water and North Atlantic Deep Water (NADW). Moving southward away from the formation region, the concentration of anthropogenic CO in NADW decreases because the older waters were exposed to lower atmospheric CO perturbations, and because of mixing with adjacent bottom waters containing little or no anthropogenic CO. In total, nearly 7 Pg of anthropogenic carbon is associated with NADW [3]. Thus, NADW contains substantially less anthropogenic CO than AAIW, even though NADW has a tremendous impact on the large-scale circulation of the ocean.

There is little anthropogenic CO associated with Antarctic Bottom Water, although exact reconstructions of the anthropogenic CO concentration in this water mass were hampered because of limited carbon data available in regions where these bottom waters are forming. The low anthropogenic CO inventories in these water masses are thought to result from a very high Revelle factor (Fig. 3), the limited contact with the surface before being transported into the ocean interior, and the physical barriers to CO uptake from the presence of sea-ice [Poisson and Chen, 1987]. In addition, the anthropogenic CO signals acquired at the surface are quickly diluted with older waters that contain no anthropogenic CO as they sink into the abyssal ocean.

Because most of the deep ocean waters have not been in contact with the atmosphere during the anthropocene [Stuiver et al., 1983], the 1994 inventory of anthropogenic CO in the ocean is only ~15% of the inventory it would have if the average surface concentration of anthropogenic CO (56 mol kg) were found throughout the ocean. This scenario, however, does not account for the Revelle factor, which makes the uptake capacity of the deep and intermediate waters much lower than that of the surface waters. Calculating the DIC increase from an 80 parts per million (ppm) change in global ocean PCO values (equivalent to the 1994 atmospheric CO increase from preindustrial) implies that the 1994 inventory is ~30% of the ocean potential at that time.

The ocean's role in the global carbon cycle. The global ocean inventory estimated here permits us, for the first time, to place observational constraints on the anthropogenic CO budget for the anthropocene. In particular, it permits us to estimate the magnitude of the time-integrated terrestrial carbon balance, which cannot be easily deduced from observations. We first consider the anthropogenic budget terms that are relatively well constrained. Over the anthropocene, about 244 ± 20 Pg C was emitted into the atmosphere as a result of the burning of fossil fuels and cement production [Marland et al., 2003] (Table 1). About two-thirds of these emissions have remained in the atmosphere, increasing the atmospheric CO concentration from about 281 ± 2 ppm in 1800 [Etheridge et al., 1996] to 359 ± 0.4 ppm in 1994 [Keeling and Whorf, 2004], which translates to an increase of 165 Pg C. Subtracting our ocean inventory estimate of 118 ± 19 Pg C and the atmospheric inventory change from the integrated fossil-fuel emissions constrains the net carbon balance of the terrestrial biosphere to be a net source of 39 ± 28 Pg C for the period between 1800 and 1994. Therefore, the ocean has constituted the only true net sink for anthropogenic CO over the past 200 years. Without this oceanic uptake, atmospheric CO would be about 55 ppm higher today than what is currently observed (~380 ppm).

Table 1

Table 1. Anthropogenic CO budget for the anthropocene (1800 to 1994) and for the decades of the 1980s and 1990s.

The terrestrial net source represents a balance between CO emissions from land-use change, and an uptake of CO by the terrestrial biosphere. Emissions from land-use change are ill-constrained. By comparing carbon storage between potential natural vegetation and present-day land cover, de Fries et al. [de Fries et al., 1999] estimated a total loss of about 180 to 200 Pg C since the mid-holocene. Using a carbon accounting model for land-use change, Houghton and Hackler [Houghton and Hackler, 2002] estimated a carbon loss of about 143 Pg C for the period from 1850 to 1994, with an uncertainty of about 50%. Extrapolating their estimate back to 1800 gives a loss of about 160 Pg C for the anthropocene. Comparisons of land-use change emissions between different estimates for the past two decades reveal, however, that Houghton and Hackler's estimates tend to be nearly twice as large as those of others [Sabine et al., 2004]. Taking this factor into account and the large uncertainty associated with these estimates, we adopt a range of 100 to 180 Pg C for land-use change emissions between 1800 and 1994. With this range, we infer that the terrestrial biosphere must have taken up between 61 and 141 Pg C from the atmosphere over the anthropocene.

It is interesting to contrast this anthropogenic CO budget over the anthropocene with that over the past two decades [Sabine et al., 2004]. Note that the emissions from fossil fuel and cement production in the decades of the 1980s and 1990s are nearly half of the anthropocene emissions (Table 1). The airborne fraction, i.e., the fraction of the combined fossil-fuel and land-use emissions that remains in the atmosphere, is statistically indistinguishable between the two periods, i.e., 39 to 48% for the anthropocene versus ~46% for 1980 to 1999 (Table 1). There is an indication, although not statistically significant, that the ocean-uptake fraction has decreased from 28 to 34% to about 26%, whereas the sink strength of the terrestrial biosphere appears to have remained constant within the large uncertainty bounds (18 to 33% versus 28%).

Future changes. On the time scales of several thousands of years, it is estimated that ~90% of the anthropogenic CO emissions will end up in the ocean [Archer et al., 1998]. Because of the slow mixing time of the ocean, however, the current oceanic uptake fraction is only about one-third of this value. Studies of the coupled carbon-climate system have suggested that on decadal time scales, the ocean may become a less efficient sink for anthropogenic CO because of positive feedbacks in the coupled carbon-climate system [Gruber et al., 2004]—consistent with the suggestion of a decreasing ocean-uptake fraction noted from Table 1.

There is a potential for both positive and negative feedbacks between the ocean and atmosphere, including changes in both the physics (e.g., circulation, stratification) and biology (e.g., export production, calcification) of the ocean. These processes are still not well understood. On the time scales of decades to centuries, however, most of the known chemical feedbacks are positive. If the surface ocean PCO concentrations continue to increase in proportion with the atmospheric CO increase, a doubling of atmospheric CO from preindustrial levels will result in a 30% decrease in carbonate ion concentration and a 60% increase in hydrogen ion concentration. As the carbonate ion concentration decreases, the Revelle factor increases and the ocean’s ability to absorb more CO from the atmosphere is diminished. The impact of this acidification can already be observed today and could have ramifications for the biological feedbacks in the future [Feely et al., 2004]. If indeed the net feedbacks are primarily positive, the required socioeconomic strategies to stabilize CO in the future will be much more stringent than in the absence of such feedbacks. Future studies of the carbon system in the oceans should be designed to identify and quantitatively assess these feedback mechanisms to provide input to models that will determine the ocean’s future role as a sink for anthropogenic CO.

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Notes

Bottle data and 1° gridded distributions are available through the GLODAP Web site (http://cdiac.esd.ornl.gov/oceans/glodap/Glodap_home.htm).

Materials and methods are available as supporting material on Science Online.

Five intermediate water masses and NADW were defined using the following temperature (T) and salinity (S) properties: Pacific AAIW: 33.8 < S < 34.5 and 2 < T < 10; NPIW: S < 34.3 and 5 < T < 12; Indian AAIW: 33.8 < S < 34.5 and 2 < T < 10; Red Sea Water: S > 34.8 and 5 < T < 14; Atlantic AAIW: 33.8 < S < 34.8 and 2 < T < 6; NADW: 34.8 < S < 35 and 1.5 < T < 4. Water mass inventories were determined by summing up the gridded anthropogenic CO values within a region defined by the T and S limits using the Levitus World Ocean Atlas 2001 salinity and temperature fields.

We thank all individuals who contributed to the global data set compiled for this project, including those responsible for the hydrographic, nutrient, oxygen, carbon, and chlorofluorocarbon measurements, and the chief scientists. The amount of work that went into collecting, finalizing, and synthesizing these data in a manner that makes a publication like this possible can never be properly acknowledged. This work was funded by grants from NOAA/U.S. Department of Energy and NSF. Partial support for K.L. was also provided by the Advanced Environmental Biotechnology Research Center at Pohang University of Science and Technology. This is Pacific Marine Environmental Laboratory contribution number 2683.

Supporting Online Material

www.sciencemag.org/cgi/content/full/305/5682/367/DC1

Materials and Methods

Fig. S1

Table S1

___________

*To whom correspondence should be addressed. Email: chris.sabine@noaa.gov

Figure Captions

Fig. 1. Column inventory of anthropogenic CO in the ocean (mol m). High inventories are associated with deep water formation in the North Atlantic and intermediate and mode water formation between 30° and 50°S. Total inventory of shaded regions is 106 ± 17 Pg C.

Fig. 2. Representative sections of anthropogenic CO (mol kg) from (A) the Atlantic, (B) Pacific, and Indian (C) oceans. Gray hatched regions and numbers indicate distribution of intermediate water masses (and North Atlantic Deep Water) on the given section and the total inventory of anthropogenic CO (Pg C) within these water masses. The southern water masses in each ocean represent Antarctic Intermediate Water. The northern water masses represent the North Atlantic Deep Water (A), North Pacific Intermediate Water (B), and Red Sea/Persian Gulf Intermediate Water (C). The two bold lines in each panel give the potential density [ = (density – 1) × 1000] contours for the surfaces shown in Fig. 4. Insets show maps of the cruise tracks used. Note that the depth scale for (A) is twice that of the other figures, reflecting the deeper penetration in the North Atlantic.

Fig. 3. Map of the 1994 distribution of Revelle factor, (PCO/ DIC)/ (PCO/DIC), averaged for the upper 50 m of the water column. A high Revelle factor indicates that, for a given atmospheric CO perturbation, the oceanic equilibrium concentration of anthropogenic CO will be lower than that for low–Revelle factor waters. The current Revelle factors are about one unit higher than they were in the preindustrial ocean.

Fig. 4. Maps of anthropogenic CO on the (A) 26.0 and (B) 27.3 potential density surfaces. Bold lines at the edge of the colored region indicate areas where the density surface outcrops. The highest values are generally observed closest to the outcrop and decrease toward the equator.

Table 1. Anthropogenic CO budget for the anthropocene (1800 to 1994) and for the decades of the 1980s and 1990s.


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