A Comparison of CO2 and 13/12C Seasonal Amplitudes in the Northern Hemisphere

T. P. WHORF, C.D. KEELING, AND M. WAHLEN

Scripps Institution of Oceanography, La Jolla, California 92093-0220

INTRODUCTION

To better understand the sources and sinks of atmospheric carbon dioxide, the Scripps Institution of Oceanography (SIO) continues to maintain cooperative programs of CO2 measurements with CMDL at Mauna Loa Observatory, Hawaii (MLO, 20°N), Point Barrow, Alaska (BRW, 71°N), Cape Kumukahi (KUM, 20°N), Samoa (14°S), and the South Pole (SPO), where air samples have been collected in 5-L glass flasks on a weekly to twice monthly basis, the latter at SPO. In addition, SIO continues to record atmospheric CO2 concentrations on a continuous basis at Mauna Loa using a non-dispersive infrared (NDIR) gas analyzer installed on site in 1958. Studies of the MLO record in the last few years include a report on changes in the rate of rise of CO2 and its relationship with global temperatures [Keeling et al., 1995].

More recently, seasonal cycle studies of data from MLO and BRW, augmented by data from Alert, N.W.T (ALT, 82°N), have been published [Keeling et al., 1996] that have yielded evidence of climate induced CO2 changes in the form of possible changes in the growth of plants on a very large spatial scale. The Alert measurements have been collected under a cooperative program between SIO and the Atmospheric Environment Service of Canada. The SIO carbon dioxide program also continues to monitor CO2 concentrations at Christmas Island (2°N), Baring Head, New Zealand (41°S), Raoul Island, Kermadec Islands (29°S), and La Jolla, California (LJO, 33°N), the last of which started in 1969 and now includes both continuous and flask measurements.

Since 1978 the 13C/12C isotopic ratio of atmospheric CO2 has been determined from the same 5-L flask samples of CO2 that have been measured for CO2 concentration. In the early years isotopic ratio was measured at MLO, SPO, and LJO and by the mid-1980s at a total of ten sites. Measurements before 1992 were determined using a VG Micromass 903 and a VG SIRA 9 mass spectrometer at the Groningen Isotopic Physics Laboratory in the Netherlands [Keeling et al., 1989]. Samples since then have been analyzed using a VG PRISM Series II mass spectrometer at SIO.

Changes in the amplitude of the seasonal cycle in CO2 concentration at MLO were first observed and reported in the early 1980s [Bacastow et al., 1985]. A more recent analysis of seasonal cycle variations observed at MLO has shown an increase in amplitude of 20% since the mid-1960s, an earlier drawdown of CO2 in the late spring and early summer by up to a week since the late 1970s, and a correlation between amplitude changes there and tempera-tures averaged over the northern hemisphere [Keeling et al., 1996]. Here we discuss seasonal changes in the 13C/12C isotopic ratio of atmospheric CO2 and how they compare with changes in amplitude of CO2 concentration.

DATA AND ANALYSIS

Measurements of 13C/12C used in this study come from the same 5-L flask samples that have all been analyzed for CO2 concentration with an NDIR analyzer of the same design as that installed at MLO. Concentrations were calibrated with our standard suite of reference gases and expressed in the X93 mole fraction scale. Air samples were rejected if pairs did not agree within 0.40 ppm of the lowest flask average (0.60 ppm at Point Barrow), if they were single analyses, or if found to be outliers having a residual greater than three sigma from our smooth curve fit. This fit, described in Keeling et al. [1989], uses four harmonics to describe the seasonal variations plus a cubic spline [Reinsch, 1967] to describe the interannual variations. A linearly-increasing gain factor was incorporated into the fitting routine when it became apparent that there were significant increases in the seasonal amplitude. This same fitting procedure has been applied to the isotopic measurements.

Isotopic data are obtained from samples of CO2 extracted cryogenically which have passed the above 0.40 or 0.60 ppm cutoff criterion. Data for MLO and BRW are shown in Figure 1 as monthly averages and expressed as the reduced isotopic ratio, 13d, of atmospheric CO2 [Keeling et al., 1989, p. 170]. Similar data have been obtained at the other SIO site locations. In 16 years of MLO 13 d isotopic data, over 700 daily samples have been analyzed amounting to approximately 44 per year, while at BRW in 14 years, some 500 daily samples have been analyzed yielding about 36 per year. Since 1992 when samples were first analyzed at SIO, gas standards have also been run daily in order to track any changes in the spectrometer output and thereby correct for them. These standards were recently calibrated against NBS19 (in 1996), to finalize calibrations begun in 1994. Along with this set of recent calibrations, a correction of +0.095 per mil was applied to all data analyzed at Groningen and previously published [Keeling et al., 1989; 1995]. This correction term is based on extensive duplicated measurements of these daily gas standards on the mass spectrometers at the Netherlands and at SIO.
 

Time trend of the reduced isotopic ratio

Figure 1. Time trend of the reduced isotopic ratio, 13d, of atmospheric CO2 in per mil difference from the international carbonate standard, PDB, for Point Barrow (BRW) and Mauna Loa (MLO). The data are shown as monthly averages and the curve by a four-harmonic fit with spline, as described.
 

RESULTS

Figures 2-4 show relative seasonal amplitudes computed annually by least-square fitting the annual function g(1 + Atm) multiplied by the four harmonics derived in the overall fit to the data of each year independently. In this expression, g denotes the annual relative amplitude, tm the midpoint time of the record, and A, a constant gain factor for the record being fit expressed in percent change in amplitude per year. The harmonic function is thus phase locked to the fit of the overall data set. Amplitudes are expressed relative to the mean annual cycle arbitrarily set at the midpoint in time of the fit [Bacastow et al., 1985]. For purposes of intercomparison between stations or different time periods, the gain factor has been afterwards adjusted to a common date (see below).
 

Comparisons of relative seasonal amplitudes for CO2 concentrations at the three most norhernly stations

Figure 2. Comparisons of relative seasonal amplitudes for CO2 concentration and 13d at the three most northerly stations (a) Alert (ALT), (b) Point Barrow (BRW) and (c) La Jolla (LJO), each referred to the midpoint of its isotopic record (open circles). The large solid circles for LJO are continuous data.

Comparisons of relative seasonal amplitudes for CO2 concentration at MLO and KUM

Figure 3. Comparisons of relative seasonal amplitudes for CO2 concentration and 13d at (a) Mauna Loa (MLO), flask data, and (b) Cape Kumukahi (KUM), each referred to the midpoint of its isotopic record (open circles). The large amplitude at KUM in 1984 is partly due to a strong shift in trend following the 1983 El Niño..
 
 

Comparison of seasonal amplitudes of CO2 concentration for MLO and KUM

Figure 4. Comparison of seasonal amplitudes of CO2 concentration for MLO (continuous data) and KUM, referred in this figure to the midpoint of the 1958-1995 Mauna Loa data. KUM amplitudes are adjusted to have the same mean as MLO amplitudes for the first 10 years of the KUM record (1979-1988).
 

Figures 2 and 3 show comparisons of seasonal amplitudes for CO2 and 13d for our northern hemisphere sites, (ALT, BRW, LJO, MLO, and KUM) in which the CO2 station data have been fit over the same time periods as there exists data for 13d, typically beginning around 1980 except for ALT data, which begins later. This is so that the relative amplitudes for the two quantities are referenced to the same times to give an optimal comparison. Though the daily averages used in the isotopic fits are not identically the same as those used in the CO2 fits, they number approximately 90% of the number for CO2, except at La Jolla where it is about 60%. In addition, the figures showing BRW, LJO, and MLO flasks have CO2 data extending back in time to before the beginning of the isotopic data. In these cases, fits to these longer records have yielded earlier CO2 relative amplitudes which have subsequently been adjusted so as to be referenced to the same time as in the shorter fit and then included in these figures. Increasing amplitudes are more apparent in these longer records. Gain factors calculated for the longer records shown at these three sites and referenced to 1970 near the start of these fits are BRW: 1.03 ± 0.16% yr-1, LJO: 1.21 ± 0.17% yr-1, and MLO flasks: 0.82 ± 0.15% yr-1. The slightly larger fluctuations before and including 1981 for LJO and MLO flasks are attributed to there being significantly fewer annual data than in the latter part of each of these records. As an exception, the LJO record includes continuous CO2 data in 1973-1975 (three large symbols) based on 5-hour averages of steady data subsequently converted to weekly data, so that these years are of significantly higher quality than other early years containing sparse flask data.

The fluctuations in 13d seasonal amplitudes occurring over several year periods show a strong tendency to follow the CO2 fluctuations during the same times, especially at BRW and LJO. A significant part of semi-decadal to decadal changes in seasonal amplitude are likely due to large scale temperature changes [Keeling et al., 1996] while other fluctuations may be a result of the effect of interannual variations connected with El Niño events. Slightly larger isotopic swings in the annual amplitudes at LJO may be partly attributable to the fewer isotopic data at this site. Comparisons of the absolute seasonal amplitudes of 13d with CO2 concentration for our northern hemisphere sites show a rate of change in 13 d with respect to CO2 of close to 0.05 per mil per ppm, as would be expected by a predominantly terrestrial component in CO2. An interesting but unexplained observation is that multi-year seasonal changes at ALT in both 13d and CO2 seem to be out of phase with changes at BRW by a couple of years, particularly near 1992.

Comparison of seasonal changes in 13d and CO2 concentration do not seem to follow each other as closely at MLO as at BRW and LJO. This may stem from part of the seasonal cycle in CO2 concentration being produced by oceanic processes that influence it without significantly affecting the amplitude of 13d. A difference in the trends of the seasonal amplitudes in concentration and 13d is also apparent at MLO as evidenced by the differing gain factors 13d and CO2.

Gain factors for CO2 concentration and 13d, compared over the same time intervals and referred to 1970, are expressed as annual rates of change in Table 1. Annual rates referred to 1980 would be about 8-10% smaller than if referred to 1970. No significant change in the seasonal cycle of 13d is apparent in the MLO flask record since 1980, whereas the increase in seasonal amplitude of CO2 concentration over the same period exceeds the standard error by more than a factor of two.

An additional observation of seasonal amplitude changes in CO2 between MLO (continuous data) and KUM (Figure 4) where respective gain factors over the same period are shown in Table 1, shows no increase in seasonal amplitude at KUM since 1979. Also, no significant increase in amplitude is evident in the isotopic data. Since KUM, situated close to sea level, supplies principally oceanic air and MLO, at 3400 m, supplies air from aloft which is better mixed, some of this difference might stem from the sampling of different sources, MLO perhaps getting a greater percentage of air which has been influenced by passage over land.

TABLE. 1. Annual Rate of Increase in the Seasonal Amplitude of

Atmospheric CO2 and 13d at Various Locations

       

Rate of 

 

Approx.

 

Inclusive Years

Increase*

Location

Latitude

Type

of Observations

(in percent)

Alert

82°N

CO2 

1985-1995

1.21 0.36

   

13d

1985-1995

2.48 0.63

         

Point Barrow

71°N

CO2 

1974-1995

1.03 0.16

   

CO2 

1982-1995

1.10 0.29

   

13d

1982-1995

0.58 0.35

         

La Jolla

33°N

CO2 

1970-1995

1.21 0.17

   

CO2 

1978-1995

1.16 0.33

   

13d

1978-1995

0.65 0.42

         

Mauna Loa

       

(flasks)

20°N

CO2 

1968-1995

0.82 0.15

   

CO2 

1980-1995

0.61 0.25

   

13d

1980-1995

-0.16 0.37

         

Mauna Loa

       

(continuous)

20°N

CO2 

1958-1995

0.62 0.04

   

CO2 

1979-1995

0.34 0.12

         

Kumukahi

20°N

CO2 

1979-1995

-0.43 0.23

   

13d

1979-1995

0.11 0.41

*With reference to January 1, 1970, except for Alert referred to January 1, 1980.

Finally, there is a hint that whatever may be causing any divergence between the trend in seasonal amplitudes of 13d and CO2 concentration at MLO may also be occurring at BRW and LJO as shown by lower gain factors for 13d over the same intervals (Table 1). These changes, however, are not significant since the isotopic records are not yet long enough to draw any firm conclusions.
 

CONCLUDING REMARKS

The SIO 13C/12C isotopic data have recently received final calibrations and have been analyzed to look for similarities and significant divergences in seasonal amplitude from the CO2 concentration data. At several northerly sites including BRW and LJO, isotopic changes in seasonal amplitude appear to track the CO2 amplitude changes quite well over periods of several years, suggesting that a dominant component in the seasonal signal of CO2 is terrestrial plant activity. At other sites such as MLO in Hawaii, differences between trends in 13d and CO2 concentration suggest an oceanic component. At this time, when subtle changes are just becoming apparent in concurrent concentration and 13C/12C records of atmospheric CO2, we hope to be able to continue these measurements, as in the case of concentration data in the early 1980s when an increase in seasonal amplitude first became apparent in our longest records.

Acknowledgments. This work was supported by Grant ATM91-21986 of the National Science Foundation, Grant DE-FG03-95ER62075 of the U.S. Department of Energy and Grant NAGW-2987 of the U.S. National Aeronautics and Space Administration. In addition, through Contract 50RANR100090, NOAA provided for the cost of maintaining our primary standard reference gases used to maintain accuracy in our measurements of atmospheric CO2. We are grateful to CMDL for providing assistance in our sampling program and for maintenance of our continuous recording instrument at MLO.
 

REFERENCES

Bacastow, R.B., Keeling, C.D., Whorf, T.P., Seasonal Amplitude Increase in Atmospheric CO2 Concentration at Mauna Loa, Hawaii, 1959-1982, J. Geophys. Res., 90, 10,529-10,540, 1985.

Keeling, C.D., Bacastow, R.B., Carter, A.F., Piper, S.C., Whorf, T.P., Heimann, M., Mook, W.G., and Roeloffzen, H., A three-dimensional model of atmospheric CO2 transport based on observed winds: 1. Analysis of observational data, in Aspects of Climate Variability in the Pacific and the Western Americas, edited by D. H. Peterson, Geophysical Monograph, American Geophysical Union, 55,165-236, Washington, DC, 1989.

Keeling, C.D., Whorf, T.P., Wahlen, M., van der Plicht, J., Interannual extremes in the rate of rise of atmospheric carbon dioxide since 1980, Nature, 375, 666-670, 1995.

Keeling, C.D., Chin, J.F.S., Whorf, T.P., Increased activity of northern vegetation inferred from atmospheric CO2 measurements, Nature, 382, 146-149, 1996.

Reinsch, C. H., Smoothing by spline functions, Numerische Mathematik, 10, 177-183, 1967.
 

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