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Showing posts with label Carbonsphere. Show all posts
Showing posts with label Carbonsphere. Show all posts

Tuesday, August 9, 2016

The Keeling Curve and Global CO2

This post is taken from a presentation which I gave at a local geologic conference in 2104, with minor modifications.


Major findings of the CO2 study:
  • Atmospheric CO2 is rising globally as a result of human activities, principally the burning of fossil fuels. 
  • Atmospheric CO2 concentration is now about 40% higher than pre-industrial CO2 concentration.
  • CO2 emissions from fossil fuels mostly originate in the Northern Hemisphere.  A global system of monitoring stations shows the dispersion of these emissions from the Northern Hemisphere to the Southern Hemisphere.
  • Atmospheric CO2 shows a seasonal cycle that is dominated by plant growth in the Northern Hemisphere.
  • The amplitude of the seasonal cycle is increasing due to human agriculture.  Agriculture accounts for about 1/3 of the seasonal cycle.
  • The Southern Hemisphere has a seasonal cycle that is the opposite polarity of the Northern Hemisphere, but is very weak due to a smaller land mass and less agriculture.
  • Atmospheric CO2 concentrations and carbon isotope ratios are changing much slower than expected if all human carbon emissions remained in the atmosphere.  About half of human carbon emissions are being absorbed by carbon reservoirs (oceans, soils and biomass).  Carbon isotopes show that large volumes of atmospheric carbon are freely exchanged with carbon in carbon reservoirs.  
  • The size of the carbon reservoirs exchanging carbon with the atmosphere can be estimated through the dilution of human-derived carbon isotopes in the atmosphere.  The calculation indicates that these carbon reservoirs contain about 7 times the quantity of carbon in the atmosphere.  This solution is about 40% larger than estimates using other methods.
  • Human carbon emissions will continue.  Forecasts indicate that atmospheric CO2 will reach 450 ppm by the year 2036.
  • After filtering the seasonal cycle from the carbon isotope data, a multi-year cycle remains.  The multi-year cycle can be correlated with the El Nino climate cycle.  The El Nino cycle changes the rate at which atmospheric carbon is absorbed by the Pacific Ocean, and changes isotopic composition of the atmosphere.



The Keeling Curve and Global CO2
S. D. Robbins                       May 15, 2014

Abstract

The Keeling Curve is a remarkable series of atmospheric CO2 measurements taken at Mauna Loa, Hawaii, from 1960 to the present.  The curve shows seasonal cycles and a steady rise in the concentration of CO2, beginning about 315 ppm and currently approaching 400 ppm.   Long-term CO2 records are also available from a number of other observatories, located from the Arctic Ocean to the South Pole.   Integration of the global dataset with carbon emissions data provides additional insights about the world’s carbon cycle. 

Atmospheric CO2 concentrations and CO2 carbon isotopes show seasonal and long term trends which vary by latitude.  The seasonal cycle is strongest in the Northern Hemisphere, and the Northern Hemisphere leads the Southern Hemisphere in terms of rising CO2.  People and plants in the Northern Hemisphere cause changes in atmospheric CO2 which propagate from the Northern Hemisphere to the Southern Hemisphere. The dispersion of CO2 from human sources can be seen as a progression through the global data.  This progressive change is seen in bulk concentration of CO2, in carbon isotopes of CO2, and the amplitude of the seasonal cycle.  Long-term changes in global CO2 are consistent with known volumes of fossil fuel emissions.   A simple model can be constructed based solely on human carbon emissions and agricultural biomass, that matches the observed seasonal cycle and long-term trends in bulk CO2,.  This model shows that it is reasonable to conclude that human activities are influencing carbon dioxide in the atmosphere.  The Energy Information Agency (EIA) predicts rising carbon emissions for the foreseeable future, from about 35 gigatonnes CO2 annually to nearly 50 gigatonnes CO2 by the year 2040, in the base-case forecast.

Carbon dioxide from fossil fuels and deforestation carries a distinctive isotopic signature, which marks the movement of man-made CO2 through the atmosphere and carbon reservoirs (soils, biomass, and oceans).  This movement of carbon, as seen in both carbon isotope data and bulk CO2 data, reveals complexity in the carbon cycle.  Discrepancies between the datasets imply the active exchange of carbon between the atmosphere and carbon reservoirs.  More than 85% of anthropogenic CO2 emissions, as tagged by carbon isotopes, do not remain in the atmosphere, but are absorbed by carbon reservoirs.  However, some of the anthropogenic carbon in the atmosphere is exchanged for natural carbon from carbon reservoirs, so that atmospheric CO2 concentration is maintained at a level equivalent to about 44% of cumulative annual CO2 emissions over the long term.  The size of carbon reservoirs is estimated at more than 7 times the volume of carbon present in the atmosphere, based on a dilution calculation of anthropogenic carbon isotopes in the atmosphere.  The role of the ocean in exchanging carbon with the atmosphere is illustrated by the correlation of atmospheric carbon isotope data with the Oceanic Niño Index (ONI), which is a measure of the El Niño/La Niña climate cycle based on sea-surface temperatures.
 

Understanding the patterns of atmospheric CO2 may provide a tool for recognizing and measuring changes in global climate.  Additional monitoring of carbon reservoirs, particularly of the world’s oceans, will be necessary to develop a comprehensive model of the earth’s carbon cycle. 


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A Few Words about CO2 Carbon Isotopes
There are two stable isotopes of carbon, C13 and C12.   C12 is the more abundant isotope; the natural ratio of C12 to C13 is about 99 to 1.  The standard measure of carbon isotopes compares the C12/C13 isotope ratio of the sample in question to the C13/C12 ratio of a standard limestone, according to the expression:

d C13/C12 = ((C13/C12 sample  / C13/C12 standard) – 1)*1000.

This expression, commonly termed “del 13”, amplifies small but meaningful differences in the isotopes, which are diagnostic of certain processes and occurrences of carbon.  The standard is a uniform Cretaceous limestone with a d 13 value defined as zero.   Positive values indicate a heavier composition, i.e., a greater concentration of C13 than the standard.  Negative values indicate a lighter composition, i.e., a smaller concentration of C13 than the standard.
Plants fractionate carbon, favoring the lighter isotope C12.  Anything derived from plants, including oil, gas, and coal (and algae, animals and people) carries a light (negative) d C13/C12 signature.  Limestone carries a d  C13/C12 ratio near zero.  The atmosphere, in 1977, had a d C13/C12 ratio of about -7.5; it is currently about -8.3, reflecting the influence of fossil fuels.  Oceans have a slightly positive d C13/C12 ratio of dissolved inorganic carbon, although Northern Hemisphere waters show a negative ratio due to the greater use of fossil fuels in the Northern Hemisphere.  Fossil fuel CO2 emissions and CO2 emissions from deforestation carry a very light d C13/C12, in the range of -25 to -28.  The distinctive isotopic signature of CO2 from fossil fuels and deforestation is useful in tracking the movement of carbon through the atmosphere and oceans.  Boden, Marland and Andres (2013) published estimates of the annual CO2 released by fossil fuels and the d C13/C12 ratio of those emissions.  Those estimates were used in this work.  

Part 1:  The Global Record

Global CO2 is rising, and the isotopic composition of atmospheric CO2 is becoming lighter.


A network of observatories, mostly operated by Scripps Oceanographic Institute, monitors global atmospheric CO2 concentrations and CO2 carbon isotopes.   Bulk CO2 has been monitored since 1957, and CO2 carbon isotopes since 1977.  In all figures, data from the Northern Hemisphere is indicated in cool colors, and data from the Southern Hemisphere is indicated with warm colors.

Global CO2 observations show a seasonal cycle and a steady rise in the concentration of CO2.  Today’s concentration of atmospheric CO2 is about 25% higher than in 1957, and about 40% higher than in 1800. 

The carbon isotope ratio (d C13/C12) of atmospheric CO2 is becoming lighter, which is consistent with the isotopic signature of fossil fuels mixing with the atmosphere.


 The amplitude of the CO2 seasonal cycle is largest in the high latitudes of the Northern Hemisphere, and diminishes southward.  The polarity of the Northern Hemisphere cycle persists to about 30 degrees South Latitude.   From that point southward, the polarity of the cycle is reversed, but with low amplitude.


Part 2:  Long Term Trends

The Northern Hemisphere leads the Southern Hemisphere in rising CO2 values and falling CO2 carbon isotope values.


The Northern Hemisphere holds 2/3 of the world’s landmass, and nearly 90% of the world’s population, fossil-fuel consumption, and agriculture.  People and plants in the Northern Hemisphere cause changes in atmospheric CO2 which propagate from the Northern Hemisphere to the Southern Hemisphere.

The seasonal cycle in bulk CO2 was removed by taking a one-year rolling average at each observatory.  The Northern Hemisphere leads the Southern Hemisphere in rising CO2.  The concentration of CO2 is highest in the Arctic, and is progressively lower by latitude to the South Pole.  The progression marks the dispersion of fossil fuel emissions from the Northern Hemisphere to the Southern Hemisphere.

The seasonal cycle in the CO2 carbon isotope ratio was removed by taking a one-year rolling average at each observatory.   The Northern Hemisphere leads the Southern Hemisphere in terms of falling d C13/C12 of CO2 (becoming isotopically lighter).  The isotopic composition of CO2 is lightest near the North Pole, and becomes progressively heavier to Antarctica.  The progression marks the dispersion of fossil fuel emissions from the Northern Hemisphere to the Southern Hemisphere.

A simple model was constructed to investigate the plausibility of the idea that human activity causes changes in atmospheric CO2.  The model begins at the global baseline CO2 concentration in 1970.  Model inputs included 60% of global fossil fuel emissions, allocated to Northern and Southern Hemispheres by GDP.  Global agricultural biomass was scaled by year to human population, and allocated to the Northern and Southern Hemispheres by population.  Volumes of carbon were converted to CO2 concentration by hemisphere, and defined the concentration at the poles.  Concentrations at intermediate latitudes were created by mixing concentrations from each hemisphere, with weighting by latitude.  The ease with which the model was created suggests that human activity is plausibly responsible for much of the change in atmospheric CO2.

Part 3:  Seasonal Cycle

The Northern Hemisphere dominates the global CO2 seasonal cycle.

The Keeling Curve is characterized by a strong seasonal cycle, dominated by the Northern Hemisphere.  The concentration of atmospheric CO2 falls during the Northern Hemisphere growing season, when land plants remove carbon from the air through photosynthesis.  The concentration of CO2 rises in the fall, winter and spring as decay returns carbon to the atmosphere as CO2.


The CO2 carbon isotope ratio d C13/C12 shows a strong seasonal cycle as a mirror image of the cycle in bulk CO2 concentration.  Land plants in the Northern Hemisphere strongly fractionate carbon isotopes.  Plants preferentially absorb C12 during the growing season, raising the d C13/C12 ratio of the atmosphere.  During decay, plants return C12 to the atmosphere, and atmospheric d C13/C12 falls.

 

Amplitude of the seasonal cycle is relatively small in the Southern Hemisphere, reflecting a smaller land mass and sparse population.  Seasonal cycles in low latitudes of the Southern Hemisphere follow the polarity of the Northern Hemisphere, but with a phase shift.  Seasonal cycles in high latitudes of the Southern Hemisphere carry the opposite polarity to the Northern Hemisphere.


Amplitude of the seasonal cycle is increasing over the past 40 years, particularly at high northern latitudes.  The increase in amplitude correlates well to the increase in human population over the past 40 years.   By inference, the increase in seasonal amplitude also correlates to a proportional increase in human agriculture.  The correlation implies that agriculture accounts for about one-third of the amplitude of the seasonal CO2 cycle. 


The polarity reversal of the seasonal cycle occurs at about 30 degrees South Latitude, near the southern boundary of the Hadley convection cell.  The atmosphere north of -30 degrees latitude contains air which is mixed with air from the Northern Hemisphere; CO2 concentrations and carbon isotopes follow the seasonal cycle of the Northern Hemisphere.  The atmosphere south of -30 degrees latitude carries the seasonal cycle of the Southern Hemisphere.  This finding suggests that additional CO2 observatories between -30 degrees and -40 degrees south latitude could monitor climate-change induced expansion of Hadley circulation, by detecting air from the Northern Hemisphere, according to the Northern Hemisphere seasonal CO2 cycle.

Part 4:  CO2 Emissions

Long-term changes in atmospheric CO2 are consistent with known volumes of human CO2 emissions.



The rate of human CO2 emissions is increasing.  Anthropogenic CO2 emissions, including deforestation, have grown from about 5 gigatonnes annually in 1900 to about 38 gigatonnes in 2009.  The greatest part of that increase occurred in the last 50 years.  
The average CO2 concentration of the Northern Hemisphere leads the Southern Hemisphere by 2.5 to 4 ppm CO2.  Net annual fossil fuel emissions in the Northern Hemisphere, converted to CO2 concentration, neatly match the difference in CO2 concentration between the hemispheres.  Deforestation, (which is more prevalent in the Southern Hemisphere) was not included in the emissions numbers, which might account for the growing discrepancy in recent years.

Despite international efforts to reduce carbon emissions, global industrial CO2 emissions are rising sharply.  According to the EIA base economic forecast, fossil fuel CO2 emissions are expected to rise 45% by the year 2040, from 33 gigatonnes to 48 gigatonnes per year.  Emissions including deforestation bring the total in 2040 to 53 gigatonnes, assuming a constant rate of deforestation from 2005 to 2040.

Global average CO2 is rising at a rate equal to about 44 percent of annual CO2 emissions, including deforestation.  The forecast of future CO2 concentrations, based on expected emissions, calls for world average CO2 to exceed 450 ppm around the year 2036.  

Part 5: The Carbonsphere

The Carbonsphere consists of atmospheric carbon and all reservoirs (ocean, biomass, and soils) freely exchanging carbon with the atmosphere.



The global mix of fossil fuels has a d C13/C12 value of about -28.  Deforestation is assumed to have a d C13/C12 value of about -25.  These contrast sharply with the atmospheric d C13/C12 value of about -8, and slightly positive oceanic d C13/C12 values.  The distinctive isotopic signature of human carbon emissions allows us to track the movement of carbon through the atmosphere, and to detect the exchange of carbon with carbon reservoirs on the earth’s surface.


A 2-year lag is required for the concentration of bulk CO2 to equilibrate from sources in the Northern Hemisphere to the Antarctic.


Differences in the behavior of bulk CO2 and CO2 carbon isotopes indicate the active role of carbon reservoirs in the ocean, plants, and soil in exchanging carbon with the atmosphere. 
Bulk carbon requires about a 2-year lag for CO2 concentration to equilibrate from the Arctic to the Antarctic.  In contrast, CO2 carbon isotopes require an 8-year lag for equilibration. 
The difference indicates that the specific molecules released by fossil fuels are cycled through carbon reservoirs and replaced in the atmosphere by other molecules from those reservoirs.  The difference in equilibration lag of bulk carbon and carbon isotopes indicates residency time in those reservoirs.

Atmospheric CO2 concentration rises at a rate equal to about 44% of human CO2 emissions, including deforestation.  If all human carbon emissions remained in the atmosphere, the concentration of atmospheric CO2 would be much higher.  

Atmospheric CO2 d C13/C12 falls at a rate incorporating about 12% of human CO2 emissions. 

If all human carbon emissions remained in the atmosphere, the concentration of atmospheric CO2 would be much higher, and the d C13/C12 isotope ratio would be much lower.  Calculations indicate that atmospheric CO2 rises at a rate equal to about 44% of human CO2 emissions.  In contrast, CO2 carbon isotopes indicate that only 12% of human carbon emissions remain in the atmosphere.  More than 85% of human carbon emissions, as tagged by carbon isotopes do not remain in the atmosphere, but are cycled into other carbon reservoirs.  At the same time, natural carbon, carrying a heavier isotopic signature, is exchanged from the carbon reservoirs, maintaining a bulk CO2 concentration accumulating at a rate of 44% of human CO2 emissions.

In the inverse of the calculation above, the d C13/C12 isotope ratio of the atmosphere shows the total volume of carbon reservoirs interacting with the atmosphere.  The calculation determines the total reservoir volume necessary to produce the observed dilution of d C13/C12 from human emissions in the air.  Carbonsphere reservoirs are assumed to be in equilibrium with the atmosphere, which is demonstrated by the relatively good fit to the solution for 30 years.  The model assumes a balance of fractionation between the carbonsphere reservoirs and the atmosphere.  The solution calls for a 6000 gigatonne carbonsphere in 1979 (including the atmosphere).  This solution is about 40% larger than estimates based on carbon inventory methods.
Part 6:  Finding Niño

The CO2 carbon isotope record can be correlated with the El Niño/La Niña climate cycle, indicating large volumes of carbon exchange between the atmosphere and the tropical Pacific Ocean.



Multi-annual cycles, or “waves” are present in the CO2 carbon isotope data after removing the seasonal cycle.  Lower amplitude but correlative waves also exist in the bulk CO2 chart.  Periods of rapidly falling d C13/C12 correspond to El Niño climatic events, suggesting variability in the rate at which the tropical Pacific Ocean takes up or releases C12 to the atmosphere.  The amplitude of the waves interrupts and sometimes reverses the secular trend, indicating that the volumes of carbon exchanged sometimes exceed the volume of human carbon emissions.



A series of mathematical operations can reduce the global CO2 isotope record to a single trace which indicates the rate at which atmospheric carbon is exchanged with the Carbonsphere.  Assuming no fractionation in the exchange process, positive values indicate a faster rate of absorption of C12 by the Carbonsphere.  Negative values indicate a slower rate of C12 absorption by the Carbonsphere.  With a slight time lag, the trace can be correlated with the Oceanic Niño Index (ONI).  The ONI is a measure of sea surface temperatures published by NOAA, indicating the prevalence of El Niño or La Niño conditions. 


The trace derived from the d C13/C12 isotope data indicates variability in the rate of exchange of C12 between the atmosphere and carbon reservoirs. That curve correlates well with the Oceanic Niño Index, a measure of the El Niño/El Niña climate cycle.  La Niña conditions, which are characterized by abnormally cool sea surface temperatures, correspond with accelerated absorption of atmospheric C12 by the ocean.  El Niño conditions, characterized by warm sea surface temperatures, correspond to decreased absorption of atmospheric C12 by the ocean. 

The quality and quantity of oceanic carbon data is weak in comparison to atmospheric CO2 data.  Oceanic carbon data is limited by a lack of continuous readings or fixed observation sites, and is strongly influenced by local biological activity.  Nevertheless, at the broadest scale, oceanic dissolved inorganic carbon is isotopically lighter in the Northern Hemisphere, reflecting the influence of fossil fuels in the Northern Hemisphere.  Improved, systematic data collection in the oceans and other carbon reservoirs will be necessary to develop a comprehensive model of the earth’s carbon cycle.
Note: Since the original poster was presented in May, 2014, I have noticed that the low d C13/C12 values are located in the Atlantic Ocean, and may be associated with the Greenland Current.  It is possible that these values reflect a natural process, such as a significant volume of glacial meltwater lowering the d C13/C12 value of the seawater.

References:
Andres, R.J., T.A. Boden, and G. Marland. 2012.  Monthly
Fossil-Fuel CO2 Emissions: Mass of Emissions Gridded by One Degree
Latitude by One Degree Longitude.  Carbon Dioxide Information Analysis
Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak
Ridge, Tenn., U.S.A.  doi: 10.3334/CDIAC/ffe.MonthlyIsomass.2012

Andres, R.J., T.A. Boden, and G. Marland. 2009.  Monthly
Fossil-Fuel CO2 Emissions: Mass of Emissions Gridded by One Degree
Latitude by One Degree Longitude.  Carbon Dioxide Information Analysis
Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak
Ridge, Tenn., U.S.A.  doi: 10.3334/CDIAC/ffe.MonthlyIsomass.2009

Andres, R.J., T.A. Boden, and G. Marland. 2012.  Annual Fossil-Fuel CO2 Emissions: Global Stable Carbon Isotopic Signature.  Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.
doi: 10.3334/CDIAC/ffe.db1013.2012

Boden, T.A., Andres, R.J., and G. Marland 2013. Global CO2 Emissions from Fossil-Fuel Burning, Cement Manufacture, and Gas Flaring: 1751-2010. Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.   

Boden, T.A., G. Marland, and R.J. Andres. 2013. Global, Regional, and National Fossil-Fuel CO2 Emissions. Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A. doi 10.3334/CDIAC/00001_V2013

Ciattaglia, L., C. Rafanelli, H. Rodriguez, and J. Araujo. 2010. Atmospheric CO2 record from continuous measurements at Jubany Station, Antarctica, in Trends Online: A Compendium of Data on Global Change, Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.

Climate Prediction Center Internet Team, 2013, ONI Index, NOAA/National Weather Service, NOAA Center for Weather and Climate Prediction , Climate Prediction Center, 5830 University Research Court, College Park, Maryland 20740.
http://www.cpc.ncep.noaa.gov/data/indices/oni.ascii.txt
http://www.nwfsc.noaa.gov/research/divisions/fe/estuarine/oeip/cb-mei.cfm
Colombo, T., and R. Santaguida. 1998. Atmospheric CO2 record from in situ measurements at Mt. Cimone. In Trends: A Compendium of Data on Global Change. Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.

Conti, J., et al, 2013.  International Energy Outlook, U. S. Energy Information Administration, Office of Energy Analysis, U.S. Department of Energy, Washington, D.C.    DOE/EIA-0484(2013)
http://www.eia.gov/forecasts/ieo/

Gaudry, A., V. Kazan, and P. Monfray. 1996. Atmospheric CO2 record from in situ measurements at Amsterdam Island. In Trends: A Compendium of Data on Global Change. Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.

Houghton, R.A. 2008. Carbon Flux to the Atmosphere from Land-Use Changes: 1850-2005. In TRENDS: A Compendium of Data on Global Change. Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.

Keeling, C.D., S.C. Piper, R.B. Bacastow, M.  Wahlen, T.P. Whorf, M. Heimann, and H. A. Meijer, Exchanges of atmospheric CO2 and 13CO2 with the terrestrial biosphere and oceans from 1978 to 2000.
I. Global aspects, SIO Reference Series, No. 01-06, Scripps Institution of Oceanography, San Diego, 88 pages, 2001.

Keeling, R.F., S.C. Piper, A.F. Bollenbacher and J.S. Walker. 2008. Atmospheric CO2 records from sites in the SIO air sampling network. In Trends: A Compendium of Data on Global Change. Carbon Dioxide Information Analysis Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak Ridge, Tenn., U.S.A.

Sieminski, A., 2013, International Energy Outlook 2013, Center for Strategic and International Studies, Washington, DC.

U.S. Energy Information Agency, Data Tables, U.S. Energy Information Agency, Office of Energy Analysis, U.S. Department of Energy, Washington D.C. data tables, 2014



Sunday, November 3, 2013

Carbon Isotopes in the Atmosphere, Part I -- How Big is the Carbonsphere?

How Big is the Carbonsphere?

The term “biosphere” is commonly used to describe all of the living creatures on earth; and the term hydrosphere is used to describe all of the water at the surface of the earth.   In the same sense,  I would like to propose a new term: “carbonsphere”, to describe the sum of carbon reservoirs freely exchanging carbon with the atmosphere.   For the purpose of modeling CO2 in the atmosphere, and understanding interactions of the atmosphere, biosphere and oceans, it is important to answer the question: “How big is the carbonsphere”?

Carbon released by burning fossil fuels is isotopically lighter and distinct from atmospheric carbon.   The distinct signature of fossil fuel emissions provide a tool for tracking the movement of carbon through the atmosphere and through reservoirs exchanging carbon with the atmosphere.  We can estimate the size of the carbonsphere, given the known volumes of fossil fuel emissions and the change in isotopic composition of the atmosphere.  The calculation makes a simplifying assumption, that there is no fractionation of isotopes during the exchanges with carbon reservoirs.  These estimates may prove useful in climate change research and modeling atmospheric CO2.
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Carbon isotopes provide an important tool for understanding the destiny of carbon emitted by burning fossil fuels.  The distinctly different isotope ratio shows us the movement of carbon in the atmosphere, oceans, the earth’s surface and biosphere.

Imagine a cup of strong coffee, and a large barrel of weak coffee.  We pour the cup into the barrel.  If we know the volume of the cup, the concentration of coffee in the cup, and the change in the concentration of coffee in the barrel, we can calculate the volume of the barrel.  The barrel may have hidden compartments and baffles, but the change from coffee in the cup will soon be seen throughout the barrel.  The simple dilution model allows us to calculate the size of the carbonsphere, based on the volume of fossil fuel emissions, the carbon isotope ratio of fossil fuels and carbon isotope measurements in the atmosphere.

Carbon isotopes on earth exist in a ratio of about  1% C13 and 99% C12.    A measure of the ratios was devised to easily represent small but meaningful differences in the isotopic composition of different materials.   The measure is d C13/12, usually called “del 13”.  This measure expresses the ratio of the stable isotopes carbon 13 and carbon 12, as compared to the C13/C12 ratio in a standard material. 

The calculation of del 13 and seasonal fluctuation of carbon isotopes are explained in my earlier blog post: http://dougrobbins.blogspot.com/2012/03/seasonal-carbon-isotope-cycles.html.

The atmosphere is constantly exchanging carbon with carbon reservoirs on land and in the ocean.   The most obvious carbon reservoirs are plants, which exchange carbon with the atmosphere through photosynthesis and decay in a seasonal cycle.   Other reservoirs include soils, plant detritus, dissolved CO2 in shallow ocean waters, etc.   These reservoirs are often called “carbon sinks”, but I prefer the term reservoirs, because the reservoirs do not simply receive carbon from the atmosphere, but also actively return carbon to the atmosphere. 

Fossil fuels have released a measurable amount of isotopically light carbon into the atmosphere. The light carbon is very useful as a tracer, showing how carbon disperses in the atmosphere and moves between the atmosphere and carbon reservoirs.   The isotopic composition of the atmosphere has changed as a result of fossil-fuel use, similar to what we have seen in bulk atmospheric CO2 in previous posts.   

Figure 1 shows the location of global monitoring stations.   The monitoring stations have been collecting bulk CO2 data since the 1950s, but only began recording carbon isotope data in the 1970s.   

 Figure 2, for reference, shows the bulk CO2 concentration, commonly called the "Keeling Curve".  We can compare the rising bulk CO2 curve to the falling carbon isotope curve shown below.

Figure 3 shows the carbon isotope record, color coded by monitoring station according to latitude, with cool colors representing the Northern Hemisphere, and warm colors in the Southern Hemisphere.    As with bulk CO2, the isotope data show a strong seasonal cyclicity resulting from plant growth and decomposition in the Northern Hemisphere.   The isotope data appear noisier than the bulk CO2 data.

The atmospheric carbon isotope data appears noisy in comparison to the graph of bulk atmospheric CO2 seen in previous posts.   We’ll simplify the problem by taking the annual global average del 13 in data available from CDIAC, the Carbon Dioxide Information Analysis Center (Andres, Boden, and Marland, 2009).   [In fact, much of the "noise" in the carbon isotope record is actually meaningful data.  We explore these variations in part 2 of this post, "CO2 Carbon Isotopes and the El  Nino Climate Cycle".

Figure 4 shows the global average isotope record, by year (R.J.Andres, T.A.Boden and G.Marland, 2009).  Andres, Boden and Marland (2012) also calculated the volume of global emissions by year and the average del 13 values of those emissions.   These data allow calculation of the expected change in atmospheric del 13, given the known annual volumes and isotope ratios of fossil-fuel emissions.  
Atmospheric del 13 declined from a value of – 7.6 in 1978 to – 8.2  in 2008, reflecting the influx of light CO2 from fossil fuels.  But the decline in del 13 is much less than would be expected if all of the fossil-fuel emissions stayed in the atmosphere.   The difference shows that light isotopes from fossil fuels are being diluted into a much larger volume of carbon.

We can use a dilution model to solve for how much carbon from fossil fuels remains in the atmosphere.   Using the known volume of fossil fuel emissions, and average del 13 ratio of those emissions, we can calculate, for each year, how much the del 13 ratio of the atmosphere should have changed.   A weighted average equation is used for the dilution model.

((Ve/Ve+Va)* d13e) +((Va/Ve+Va)* d13a )  = Vna* d13n

Where:
Ve = Volume of Emissions
Va = Volume of Atmosphere
Vna = New Volume of Atmosphere
d13e = d C13/C12 of Emissions
d13a = d C13/C12 of Atmosphere
d13na = New d C13/C12 of Atmosphere

If all of the carbon from fossil fuel emissions remained in the atmosphere, the del 13 ratio of the atmosphere would have declined to  – 12 by 2008.  If about 60% of fossil-fuel emissions remained in the atmosphere, the del 13 ratio would be about – 10.  But the dilution model shows a fit to the observed average atmospheric del 13 trend when only about 14% of fossil fuel emissions remain in the atmosphere, yielding a del 13 value of – 8.2 in 2008.  This value is in marked contrast to the data for bulk CO2 composition, which indicates that 60% of fossil-fuel emissions remain in the atmosphere over the time range of our observations.  

Carbon isotope data show that the picture is complicated.  Isotopes ratios show that the greater part of fossil-fuel emissions are exchanged with other earth systems, while bulk CO2 levels seem to show a much larger retention of fossil fuel emissions in the atmosphere.   The process involves exchange and displacement.  As fossil fuel emissions are absorbed by carbon reservoirs,  other carbon is displaced, and enters the atmosphere to maintain equilibrium.   The specific molecules released by fossil fuels exchange places with carbon in carbon reservoirs, and atmospheric CO2 continues to rise.
  
Let’s look at some of the isotope data, and then consider the size of the carbonsphere.

The volume of fossil fuel emssions is known, and about 60% of fossil fuel emissions appears to accumulate in the atmosphere.   [The percentage would be somewhat lower, if carbon from burning forests is included in the calculation.]  We can calculate the expected change in del 13 based on the volume of fossil fuel CO2 emissions, and compare this figure to the observed isotopic change in the global average del 13.  

Between 1979 and 2008, 194 Gigatonnes of carbon (=710 Gt CO2) was released to the atmosphere by burning fossil fuels and manufacturing cement.   The weighted average del 13 ratio of these emissions was -28.4, reflecting the very light isotopic composition of most fossil fuels.  The atmosphere in 1979 contained about 3 1/2 times that volume of carbon, 718 Gt (=2634 Gt CO2), with an average del 13 of -7.6.  

If we assume that 60% of the fossil fuel emissions remain in the atmosphere, and run a simple mixing calculation, we conclude that the del 13 ratio of the atmosphere should have declined to about -12, a change in del 13 of -4.4.   Instead, we see a decline of only -0.7, from the initial value of -7.6 in 1979 to a value of -8.3 in 2008.   Looking at the thirty-year history of carbon isotope observations, we can calculate that only about 14% of the carbon released by fossil-fuel emissions remains in the atmosphere, by matching the results of a mixing model to the observed decline in global del 13.   The rest of the fossil-fuel carbon is diluted into a much larger reservoir of carbon than the atmosphere. 

Figure 5 shows the expected change in del 13, based on varying models of fossil fuel emissions remaining in the atmosphere.   The isotope ratio shows that only 14% of fossil fuel emissions remain in the atmosphere.
I’m going to coin a term, and call the sum of all carbon reservoirs freely exchanging carbon with the atmosphere, within an annual time-frame, the Carbonsphere.  The Carbonsphere includes the atmosphere, all plants and animals on earth (including you), dissolved carbon in the shallow ocean, weathering surfaces on limestones, coral reefs, seashells and limestone precipitating directly in the ocean.   The Carbonsphere does not include limestone below the weathering surface or carbon in the deep oceans.  These do not participate in the annual exchange of carbon with the atmophere.

With the same data used above, we can solve the inverse problem: what is the volume of reservoirs exchanging carbon with the atmosphere?  It is a dilution problem, described by the coffee analogy in the introduction.  We know the volume of fossil fuel emissions, the isotopic composition of those emissions, and the isotopic change in the atmosphere.  We can find the volume of the carbonsphere by the dilution of fossil fuel emissions.  (Note, this calculation assumes negligible fractionation of carbon isotopes during exchange with carbon reservoirs.)

Figure 6 shows a set of models, assuming a range of sizes for the carbonsphere.    The best match shows a carbonsphere of about 5200 gigatonnes in 1977.  There is fluctuation in the isotopic composition of the atmosphere which does not match the model, which we will explore in the next blog post.   The initial model of 1500 Gt is about twice the carbon volume of the atmosphere.  Over time, for the past 40 years, a carbonsphere of about 5200 gigatonnes is required to quantitatively match the dilution of the global average isotopic composition of the atmosphere.  
Estimates for the size of carbon reservoirs are available from a variety of sources.   Estimates are generated by estimating the carbon inventory for the atmosphere, land vegetation, soil, plant detritus, ocean biomass, and carbon dissolved in surface waters of the ocean.  There is a considerable range in the estimates for individual reservoirs, but general agreement about the total.  
Here is a sampling of estimates, randomly selected from the Internet: 
Traeger, C., 2009                                             3555 Gt  
Falkowski, 2000                                               3390 Gt
World Ocean Review, 2013                              3797 Gt
Corrosion Doctors                                            3000 Gt
Wheeling Jesuit University                                  3675 Gt
US Climate Change Program                             4918 Gt
CDIAC (2012)                                                 3948 Gt                                                                
All of these estimates are less than the result (5200 Gt) produced by calculating dilution of del 13 from fossil fuel emissions. 

We can speculate about the discrepancy between the results of the dilution calculation, and those obtained by making a carbon inventory.   One possibility is that the atmosphere is not in equilibrium with the carbonsphere, i.e., that isotopically light carbon from fossil fuel emissions is tied up in reservoirs near the point of emission.  Thus, there is a transient effect, a lag before the equilibration of the emissions and the atmosphere.   We will see some evidence of this in the second part of this article.   Secondly, it may be that there is a greater dispersion of carbon in the ocean than estimated in the carbon inventory.  We will see some evidence of that, also, in the second part of this article.   But for the moment, the conclusion of this work is that the carbonsphere – the sum of all carbon reservoirs freely exchanging carbon with the atmosphere – is larger than previous estimates.

I should note that these data and calculations include only fossil-fuel emissions and making cement.   The emissions volumes and del 13 averages do not include carbon released through changes in land use, principally clearing forests for agriculture by burning.  Addition carbon from burning forests is also isotopically light.  If carbon from changes in land use is included in the calculations, we would see that an even smaller percentage of carbon emissions remain in the atmosphere, and the calculated size of the carbonsphere would be even larger.

Conclusions:
1)  Isotopically light CO2 released by burning fossil fuels provides a tool for tracking movements of carbon through the earth’s systems, and for calculating the size of carbon reservoirs exchanging carbon with the atmosphere.

2)  Carbon isotope ratios show that the percentage of carbon remaining in the atmosphere from fossil fuel emissions is about 14% of those emissions.  This is in marked contrast with estimates based on bulk atmospheric CO2, which indicate that 60% of fossil fuel emissions remain in the atmosphere.   The difference is due to the exchange of carbon between the atmosphere and carbon reservoirs on the earth’s surface.

3)  The Carbonsphere can be defined as the sum of all reservoirs freely exchanging carbon with the atmosphere.   The size of the Carbonsphere can be calculated, based on the observed dilution of the del 13 carbon ratio.   The calculated size of the carbonsphere is about 5200 gigatonnes.  This estimate is substantially larger than published estimates of the size of carbon reservoirs interacting with the atmosphere.   Sources of error might include disequilibrium of the atmosphere with carbon reservoirs near the source of fossil fuel emissions, resulting in an overestimate of the size of the reservoirs diluting the fossil fuel emissions.

This study could be improved by incorporating data for emissions relating to land use.    
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References:
Annual  Isotope Global Average:
Andres, R.J. T.A. Boden, and G. Marland. 2009.  Monthly
Fossil-Fuel CO2 Emissions: Mass of Emissions Gridded by One Degree
Latitude by One Degree Longitude.  Carbon Dioxide Information Analysis
Center, Oak Ridge National Laboratory, U.S. Department of Energy, Oak
Ridge, Tenn., U.S.A.  doi: 10.3334/CDIAC/ffe.MonthlyIsomass.2009

Global Emissions average isotope data:
Andres, R.J., Boden, T.A, and Marland, G., 2012

Previous posts om this site regarding atmospheric CO2:
2)  The Keeling Curve and Seasonal Carbon Cycles
3)   Seasonal Carbon Isotope Cycles
4)   Long-Term Trends in Atmospheric CO2
5)   Modeling Global CO2 Cycles
6)   The Keeling Curve Summary:  Seasonal CO2 cycles and Global CO2 Distribution
       http://dougrobbins.blogspot.com/2013/05/the-keeling-curve-seasonal-co2-cycles.html
8)   Carbon Isotopes in the Atmosphere, Part II
       Finding Niño -- Correlation CO2 Carbon Isotopes in the Atmosphere with the El Niño Cycle
        http://dougrobbins.blogspot.com/2013/11/carbon-isotopes-in-atmosphere-part-ii.html