Academies Internship Information  Sign up for PNAS Online eTocs
Link: Info for AuthorsLink: Editorial BoardLink: AboutLink: SubscribeLink: AdvertiseLink: ContactLink: Sitemap Link: PNAS Home
Proceedings of the National Academy of Sciences
Link: Current Issue "" Link: Archives "" Link: Online Submission ""  Link: Advanced Search

Published online on March 19, 2002, 10.1073/pnas.022055499
PNAS | April 2, 2002 | vol. 99 | no. 7 | 4167-4171


This Article
Right arrow Abstract Freely available
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a colleague
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Similar articles in PubMed
Right arrow Alert me to new issues of the journal
Right arrow Add to My File Cabinet
Right arrow Download to citation manager
Right arrow Request Copyright Permission
Citing Articles
Right arrow Citing Articles via HighWire
Right arrow Citing Articles via CrossRef
Right arrow Citing Articles via ISI Web of Science (15)
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Rothman, D. H.
Right arrow Search for Related Content
PubMed
Right arrow PubMed Citation
Right arrow Articles by Rothman, D. H.
GeoRef
Right arrow GeoRef Citation
Social Bookmarking
 Add to CiteULike   Add to Complore   Add to Connotea   Add to Del.icio.us   Add to Digg  
What's this?

 Previous Article  | Table of Contents |  Next Article 

Geology
Atmospheric carbon dioxide levels for the last 500 million years

Daniel H. Rothmandagger

Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139

Communicated by Paul F. Hoffman, Harvard University, Cambridge, MA, January 30, 2002 (received for review October 9, 2001)


    Abstract
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

The last 500 million years of the strontium-isotope record are shown to correlate significantly with the concurrent record of isotopic fractionation between inorganic and organic carbon after the effects of recycled sediment are removed from the strontium signal. The correlation is shown to result from the common dependence of both signals on weathering and magmatic processes. Because the long-term evolution of carbon dioxide levels depends similarly on weathering and magmatism, the relative fluctuations of CO2 levels are inferred from the shared fluctuations of the isotopic records. The resulting CO2 signal exhibits no systematic correspondence with the geologic record of climatic variations at tectonic time scales.


    Introduction
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

The long-term carbon cycle is controlled by chemical weathering, volcanic and metamorphic degassing, and the burial of organic carbon (1, 2). Ancient atmospheric carbon dioxide levels are reflected in the isotopic content of organic carbon (3) and, less directly, strontium (4) in marine sedimentary rocks; the former because photosynthetic carbon isotope fractionation is sensitive to CO2 levels, and the latter because weathering and degassing are associated with extreme values of the abundance ratio 87Sr/86Sr. However, attempts to use these geochemical signals to estimate past CO2 levels (5-8) are hindered by the signals' additional relationships to various tectonic (9, 10) and biological (11) effects. Moreover, the strontium signal has proven especially difficult to parse (12-15).

Here, I attempt to resolve these ambiguities in the isotopic signals of carbon and strontium. First, it is shown that the last 500 million years of the strontium signal, after transformation to remove the effects of recycled sediment (16, 17), correlate significantly with the concurrent record of isotopic fractionation between inorganic and organic carbon (3). This empirical result is supplemented by the theoretical deduction that the two records are linked by their common dependence on rates of continental weathering and magmatic activity. The assumption that CO2 levels fall with the former and rise with the latter then indicates that an appropriate average of the two records should reflect the long-term fluctuations of the partial pressure of atmospheric CO2. The CO2 signal derived from this analysis represents fluctuations at time scales greater than about 10 million years (My). Comparison with the geologic record of climatic variations (18) reveals no obvious correspondence.


    Strontium and Carbon Isotopic Signals
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

Fig. 1 shows the strontium and carbon isotopic signals for the last 500 My. The data for the strontium isotope ratios 87Sr/86Sr were compiled by Veizer et al. (4) and Walter et al. (19); the former source accounts for all 87Sr/86Sr data younger than 520 My, whereas the latter was used for data extending back to 608 My (not shown). Both sets of 87Sr/86Sr data were first averaged in nonoverlapping time windows of 10 My. The resulting unevenly spaced record was then transformed (20) to an evenly spaced record with time increments of approximately 10 My and no contributions to the power spectral density at periods less than 21 My.



View larger version (22K):
[in this window]
[in a new window]
 
Fig. 1.   Data for varepsilon toc (red filled circles) (3) and 87Sr/86Sr (blue open squares) (4). The time scale for varepsilon toc has been revised from the original to match the scheme (32) used for the strontium data. The capital letters correspond to the following geologic periods: Ordovician, Silurian, Devonian, Carboniferous, Permian, Triassic, Jurassic, Cretaceous, and Tertiary.

The second record in Fig. 1, compiled by Hayes et al. (3) derives from the isotopic composition of marine organic carbon and carbonate carbon. From isotopic abundance ratios Rx = (13C/12C)x for carbon in sample x, the isotopic fractionation between sample x and a standard (STD) sample, delta x = 1,000[(Rx - RSTD)/RSTD], is obtained for carbonate (delta a) and organic (delta o) carbon. The isotopic fractionation varepsilon toc between total organic carbon and sedimentary carbonates is then given approximately by varepsilon toc = delta a - delta o, which is the second signal plotted in Fig. 1.

Fig. 1 shows a surprising similarity between the two records for fluctuations with periods less than about 100 My. However, the correlation between the two time series is not statistically significantDagger [Spearman rank correlation coefficient (21) Rs = -0.40, P = 0.17, N = 46], because the longer-period fluctuations are not in phase. It is therefore interesting to ask why the two records appear similar at shorter time scales and dissimilar at longer time scales.

Recent work has shown that the measurements of varepsilon toc approximately fit the empirical relation (3, 22)
ϵ<SUB><UP>toc</UP></SUB>=ϵ<SUB>0</SUB>−&Ggr;&cjs1134;&PHgr;. [ 1 ]
The parameter varepsilon 0 represents the isotopic effects of photosynthesis and secondary biological processes along with the isotopic depletion of dissolved CO2 in surface waters relative to sedimentary carbonate. Because varepsilon 0 is approximately constant throughout the period plotted in Fig. 1, the main source of varepsilon toc's fluctuations is contained in isotopic effects due to changing algal physiology---the permeability, surface-to-volume ratio, and growth rate of algal cells---represented by Gamma , and the concentration Phi  of dissolved carbon dioxide in surface waters (3, 8).

Although the mechanisms responsible for the fluctuations of s = 87Sr/86Sr are subject to much debate (4, 9, 10, 12-15), some aspects of the signal's evolution are nevertheless clear. Because 87Rb decays to 87Sr with a half-life of ~48 billion years, the supply of 87Sr may be taken to be approximately constant over the last 500 My. However, it is not uniformly distributed: the fluvial input to the oceans is derived in part from rocks---both silicates and metamorphosed carbonates (12-15)---that are relatively enriched in radiogenic Sr (s sime  0.712 or greater) compared to the nonradiogenic Sr of mantle origin supplied at hydrothermal vents (s sime  0.7035) (23). The value of s(t) at some particular time t represents, to first approximation, the relative fluxes of these two extreme values.

However, this first approximation ignores the recycling of rocks in the sedimentary cycle (16). As pointed out by Brass (17), about 75% of the strontium input to the oceans should come from the weathering of exposed carbonates of marine origin. Because these carbonates retain a memory of s at the time of deposition, their contribution to sedimentary Sr significantly damps the signal coming from hydrothermal vents (low s) and rocks containing radiogenic Sr (high s) (9).

Denoting the fluvial flux of radiogenic Sr by r, the input from hydrothermal vents by vh, and the memory effect by m, a simple expression for the strontium isotope ratio s is
s=&mgr;m+(1−&mgr;)g(r, v<SUB>h</SUB>), [ 2 ]
where 0 <=  µ <=  1 is the fraction of sedimentary Sr deriving from the memory flux, and g is a function that depends on both r and vh. The memory term can be approximated by assuming that sedimentary strontium is weathered at a rate proportional to its mass (16). Then m(t) is simply a weighted (exponentially decaying) average of s(tau ), tau  < t (17), which we express by the convolution
m(t)=<LIM><OP>∫</OP><LL><UP>−</UP>∞</LL><UL>t</UL></LIM> &lgr;e<SUP><UP>−&lgr;</UP>(t−&tgr;)</SUP>s(&tgr;)<UP>d</UP>&tgr;. [ 3 ]
The parameter lambda  is related to the half-life t1/2 of sedimentary Sr; i.e., lambda  = -(ln 2)/t1/2. Brass estimates 57 My < t1/2 < 102 My (17). Therefore, the memory effect should strongly influence the fluctuations of s at long time scales (greater than about 100 My), whereas the short time scale fluctuations should be relatively unaffected.

The short-time correlations may be explained in part by noting the common dependence of varepsilon toc and g on the global weathering rate w (i.e., the flux of all weathered products from the continents to the oceans) and the rate of magmatic activity v associated not only with the hydrothermal flux vh but also with volcanic degassing. Assuming that r = r(w) and vh = vh(v), g's dependence on w and v may be written§
g=g(r(w), v<SUB>h</SUB>(v)). [ 4 ]
With respect to varepsilon toc, the physiological term Gamma  may likewise depend on w because of changing nutrient concentrations in the oceans. Gamma  could also depend on CO2 levels, which in turn depend on degassing, weathering rates---because of the net uptake rate u = u(w) of atmospheric CO2 associated with silicate weathering (1, 2, 24)---and other processes, such as organic carbon burial, which we collectively designate by b. Aggregating these dependencies then yields
ϵ<SUB><UP>toc</UP></SUB>=ϵ<SUB>0</SUB>−<FR><NU>&Ggr;(w, &PHgr;(u(w), v, b))</NU><DE>&PHgr;(u(w), v, b)</DE></FR>. [ 5 ]
Comparison of Eqs. 4 and 5 directly reveals the joint dependence of g and varepsilon toc on v and w.


    Removal of the Effects of Sedimentary Recycling
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

Because the strontium signal s contains a memory effect, whereas varepsilon toc does not, removal of the memory effect should reveal correlations between s and varepsilon toc at both short and long time scales, thereby confirming the joint dependence on v and w. To test this hypothesis, I first assume it is true and use it to estimate g. For a given lambda  and µ, m is calculated by discretizing Eq. 3 for tau  > -608 My. Eq. 2 is then solved for g:
g<SUB>&lgr;&mgr;</SUB>=<FR><NU>s−&mgr;m<SUB>&lgr;</SUB></NU><DE>1−&mgr;</DE></FR>. [ 6 ]
Here the subscripts make explicit the dependencies on lambda  and µ.

Let Rlambda µ(varepsilon toc, glambda µ) be the Pearson product-moment correlation coefficient (21) that quantifies the similarity of varepsilon toc and glambda µ. From the foregoing argument, the best estimate of lambda  and µ should be that which minimizes Rlambda µ (because the expected correlation is negative). Fig. 2 shows contours of R as a function of µ and t1/2 -(ln 2)/lambda . The minimum Rlambda µ = -0.81 occurs at t1/2 = 54 My and µ = 0.99. However, the corresponding estimate of glambda µ includes values below the hydrothermal minimum of 0.7035. Such nonphysical ratios probably derive from the amplification of any measurement noise resulting from division by the small quantity - µ in Eq. 6. Indeed, the dark gray region in Fig. 2 indicates that all such results occur only for µ close to unity. I therefore define the best estimates lambda *, µ* of lambda , µ by minimizing Rlambda µ subject to the constraint that glambda µ > 0.7035. One then finds t*1/2 = -ln 2/lambda * = 41 My and µ* = 0.83, corresponding to Rlambda *µ* = -0.80 (within 1% of the unconstrained minimum). These results are in reasonable accord with Brass's estimate of the half-life of sedimentary Sr (57 - 102 My) (17) and his conclusion that "strontium leached from limestones is about 75% of the total input" (17).



View larger version (27K):
[in this window]
[in a new window]
 
Fig. 2.   Contours of Rlambda µ as a function of µ, the fraction of sedimentary Sr deriving from the memory flux, and t1/2 = -(ln 2)/lambda , the half-life of sedimentary Sr. R was calculated for µ = 0, 0.01, ... , 0.99 and t1/2 = 1, 2, ... , 99 My. For large half-life, the contours decrease from left to right as follow: -0.60, -0.65, -0.70, -0.75, -0.79. The symbol × marks the minimum, Rlambda *µ* = -0.80, obtained under the constraint that g(t) > 0.7035. The area shaded dark gray on the right does not satisfy the constraint. The rectangular area labeled "Brass" corresponds to previous estimates obtained by geochemical arguments (17); its horizontal extent has not been explicitly computed.

Fig. 3 shows glambda *µ* compared to varepsilon toc. Compared with Fig. 1, one sees that both the long and short period fluctuations are now not only approximately equally correlated, but the correlation is also significant (Rs = -0.74, P < 10-3, N = 46). The hypothesis that recycled sediment partially obscured an inherent correlation because of a shared dependence on weathering and volcanic processes is therefore confirmed.



View larger version (22K):
[in this window]
[in a new window]
 
Fig. 3.   The function g (blue squares) obtained by removing the memory flux from the 87Sr/86Sr data of Fig. 1, along with varepsilon toc (red circles). Note that the range of the 87Sr/86Sr curve is approximately five times greater than in Fig. 1. The data are plotted such that the mean of both time series lies on the same horizontal line and their rms fluctuations have the same vertical extent.


    Relationship to CO2 Levels
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

To understand further the correlation, I make the following assumptions concerning the functional dependencies contained in Eqs. 4 and 5:
<UP>d</UP>r&cjs1134;<UP>d</UP>w>0, <UP>d</UP>u&cjs1134;<UP>d</UP>w>0, <UP>and d</UP>v<SUB>h</SUB>&cjs1134;<UP>d</UP>v>0. [ 7 ]
The first two state that the flux of radiogenic Sr to the oceans and the uptake of atmospheric CO2 because of silicate weathering increase as the global weathering rate (of all minerals in all terranes) increases. The third formalizes the natural assumption that the hydrothermal flux of Sr varies with the same sign as all magmatic processes.

Because the Sr isotope ratios increase with increasing r (i.e., partial g/partial r > 0) and decrease with increasing vh (i.e., partial g/partial vh < 0), one has
<FR><NU>∂g</NU><DE>∂v</DE></FR>=<FR><NU>∂g</NU><DE>∂v<SUB>h</SUB></DE></FR> <FR><NU><UP>d</UP>v<SUB>h</SUB></NU><DE><UP>d</UP>v</DE></FR><0 <UP>and </UP><FR><NU>∂g</NU><DE>∂w</DE></FR>=<FR><NU>∂g</NU><DE>∂r</DE></FR> <FR><NU><UP>d</UP>r</NU><DE><UP>d</UP>w</DE></FR>>0. [ 8 ]
Because g and varepsilon toc are negatively correlated, one expects that varepsilon toc depends on v and w in the opposite sense:
∂ϵ<SUB><UP>toc</UP></SUB>&cjs1134;∂v>0 <UP>and</UP> ∂ϵ<SUB><UP>toc</UP></SUB>&cjs1134;∂w<0. [ 9 ]
The inequalities 8 and 9 have been obtained without making any explicit assumption concerning any dependence of r on u nor Gamma  on v and w. Because they show that v and w each influence g and varepsilon toc with opposite signs, the relative fluctuations of any other quantity that also depends on v and w with opposite signs may be inferred from the shared fluctuations of g and varepsilon toc. Specifically, the concentration Phi  of oceanic CO2 responds positively to v while its response to weathering is negative:
<FR><NU>∂&PHgr;</NU><DE>∂v</DE></FR>>0 <UP>and</UP> <FR><NU>∂&PHgr;</NU><DE>∂w</DE></FR>=<FR><NU>∂&PHgr;</NU><DE>∂u</DE></FR> <FR><NU><UP>d</UP>u</NU><DE><UP>d</UP>w</DE></FR><0. [ 10 ]
Thus the shared fluctuations of g and varepsilon toc indicate the relative fluctuations of ancient CO2 levels.||


    Estimation of the CO2 Signal
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

I proceed to estimate the CO2 signal explicitly. First, the highest measurement of varepsilon toc, at -175 My, is dropped because of its statistical insignificance (3). I then transform g(t) right-arrow varepsilon g(t), a strontium-derived estimate of varepsilon toc, by mapping the left axis of Fig. 3 to the corresponding value on the right axis. The quantities varepsilon toc and varepsilon g are then averaged to obtain
&zgr;(t<SUB>i</SUB>)=[ϵ<SUB>g</SUB>(t<SUB>i</SUB>)+ϵ<SUB><UP>toc</UP></SUB>(t<SUB>i</SUB>)]&cjs1134;2. [ 11 ]
The times ti are given by the points where varepsilon toc is specified and varepsilon g(ti) is obtained by linear interpolation. Here it is implicitly assumed that varepsilon toc and varepsilon g contain a common signal that is enhanced by averaging. Statistical arguments suggest that zeta 's rms signal-to-noise ratio lies between about 2 and 3.**

Assume now that Gamma  and varepsilon 0 are constant and define the dimensionless CO2 concentration phi  = Phi varepsilon 0/Gamma (8). In terms of phi  and zeta , Eq. 1 then yields
&phgr;(t)=<FR><NU>ϵ<SUB>0</SUB></NU><DE>ϵ<SUB>0</SUB>−&zgr;(t)</DE></FR>. [ 12 ]
At long time scales such that the oceans are in equilibrium with the atmosphere, the partial pressure pCO2 is proportional to phi  (1). The relative fluctuations of pCO2 are therefore given by phi (t)/phi (0), which is plotted in Fig. 4 for varepsilon 0 = 36 per mil (per thousand ). The gray area surrounding the pCO2 curve in Fig. 4 brackets this result for varepsilon 0 = 35per thousand and 38per thousand , a range consistent with previous estimates (3).



View larger version (23K):
[in this window]
[in a new window]
 
Fig. 4.   Fluctuations of pCO2 for the last 500 My, normalized by the estimate of pCO2 obtained from the most recent value of zeta . The solid line is obtained from Eq. 12 by using varepsilon 0 = 36per thousand . The lower and upper limits of the gray area surrounding the pCO2 curve result from varepsilon 0 = 38 and 35per thousand , respectively. The gray bars at the top correspond to periods when Earth's climate was relatively cool; the white spaces between them correspond to warm modes (18).

Fig. 4 reveals that CO2 levels have mostly decreased for the last 175 My. Prior to that point they appear to have fluctuated from about two to four times modern levels with a dominant period of about 100 My. The decline for the last 175 My is also present in several previous pCO2 reconstructions (7, 8, 26, 27), and the entire curve displays some similarity to a previous estimate derived from the geologic record of carbonate formation (26). Although the period before -175 My differs substantially from previous geochemical model calculations (7), an approximate error estimate lends considerable credence to the pCO2 curve of Fig. 4. Specifically, phi  should inherit zeta 's signal-to-noise ratio of 2-3. This correspondence would be exact if phi (zeta ) were linear. Because phi (zeta ) is monotonic for the observed range of zeta , its nonlinearity does not affect the timing of the maxima and minima of the pCO2 curve. Thus the linear error estimate remains pertinent.


    Comparison with the Climate Record
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

Using a variety of sedimentological criteria, Frakes et al. (18) have concluded that Earth's climate has cycled several times between warm and cool modes for roughly the last 600 My. Recent work by Veizer et al. (28), based on measurements of oxygen isotopes in calcite and aragonite shells, appears to confirm the existence of these long-period (~135 My) climatic fluctuations. Changes in CO2 levels are usually assumed to be among the dominant mechanisms driving such long-term climate change (29).

It is therefore interesting to ask what, if any, correspondence exists between ancient climate and the estimate of pCO2 in Fig. 4. The gray bars at the top of Fig. 4 correspond to the periods when the global climate was cool; the intervening white space corresponds to the warm modes (18). The most recent cool period corresponds to relatively low CO2 levels, as is widely expected (30). However, no correspondence between pCO2 and climate is evident in the remainder of the record, in part because the apparent 100 My cycle of the pCO2 record does not match the longer climatic cycle. The lack of correlation remains if one calculates the change in average global surface temperature resulting from changes in pCO2 and the solar constant using energy-balance arguments (7, 26).

Superficially, this observation would seem to imply that pCO2 does not exert dominant control on Earth's climate at time scales greater than about 10 My. A wealth of evidence, however, suggests that pCO2 exerts at least some control [see Crowley and Berner (30) for a recent review]. Fig. 4 cannot by itself refute this assumption. Instead, it simply shows that the "null hypothesis" that pCO2 and climate are unrelated cannot be rejected on the basis of this evidence alone.


    Discussion and Conclusion
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

One of the principal contributions of this study is methodological. From observations of a weak correlation between strontium and carbon isotopic signals (Fig. 1) and their shared dependence on global weathering rates and magmatic activity, weathering and magmatism are deduced to be the main processes driving the signals' fluctuations. Correction for the effects of sedimentary recycling enhances the correlation (Fig. 3), indicates a strong shared signal, and strengthens this conclusion.

A second, crucial step is to note that any quantity with a similar joint dependence on weathering and magmatic processes may be expected to display similar fluctuations. Here attention has been focused on CO2 levels; as for the strontium and carbon isotopic signals, CO2 levels depend on weathering and magmatism with opposite signs and should therefore fluctuate roughly in sync with the isotopic signals. Because the reasoning is general, it need not be limited to CO2. Among the many possible applications, the case of oceanic phosphate concentrations is particularly interesting. Phosphate concentrations should increase with weathering and decrease with hydrothermal activity (31); thus the methodology in this paper may be applicable to their reconstruction. Moreover, because phosphorus is a limiting nutrient, oceanic productivity may be expected to covary positively with its concentration in seawater, suggesting that CO2 levels and productivity covary negatively at geologic time scales (8).

Such reasoning naturally raises the issue of cause and effect. This study indicates that degassing and silicate weathering were the primary controls on the carbon cycle for the last 500 My. But the results do not themselves indicate whether either of these mechanisms dominated, or whether weathering was driven by the diversification of land plants (8), continental collisions (9), or a complex combination of tectonic, biological, and geochemical processes (7). They do, however, offer a new view of the long-term fluctuations of pCO2 that will hopefully stimulate novel approaches to the study of biogeochemical cycles at evolutionary time scales.


    Acknowledgements

I thank O. Aharonson, L. Derry, J. Hayes, P. Hoffman, A. Knoll, L. Kump, J. Sachs, R. Summons, and the late John Edmond for helpful remarks. This work was supported in part by National Science Foundation Grant DEB-0083983.


    Abbreviation

My, million years.


    Footnotes

dagger E-mail: dan{at}segovia.mit.edu.

Dagger Correlations between varepsilon toc(t) and s(t) or g(t) are computed from the N equal-time pairs obtained after linearly interpolating the Sr signal so that it is sampled at the same times as varepsilon toc. The statistical significance P is one-sided and was estimated by using the Monte Carlo technique described in ref. 8.

§ Although w and v could conceivably depend on one another, here such dependencies are assumed to be insignificant compared to any independent variations.

One also requires that if changes in v or w dominate one process then they dominate all processes.

|| Because Phi  can also depend on other processes b such as organic carbon burial, the shared fluctuations of g and varepsilon toc do not necessarily reflect the full evolution of Phi  but rather the "partial" contribution of v and w alone. However, the good correlation of Fig. 3 indicates that b's influence on Phi 's fluctuations has been small, except possibly in the Carboniferous. Thus one may conclude that the fluctuations of g and varepsilon toc follow to good approximation the fluctuations of Phi  with opposite signs.

** To estimate the signal-to-noise ratio of the time series zeta (t) defined by Eq. 11, assume that varepsilon toc and varepsilon g are each composed of a shared but unknown signal z in the presence of zero-mean noise eta toc and eta g, respectively: varepsilon toc = z + eta toc and varepsilon g = z + eta g. The quantity zeta  is an estimate of z. Its signal-to-noise ratio may be computed under the assumption that eta toc and eta g each have variance sigma <UP><SUB>&eegr;</SUB><SUP>2</SUP></UP>, z has variance sigma <UP><SUB><IT>z</IT></SUB><SUP><IT>2</IT></SUP></UP>, and eta toc, eta g, and z are each uncorrelated to the other. The expectation of the correlation coefficient R is then sigma <UP><SUB><IT>z</IT></SUB><SUP><IT>2</IT></SUP></UP>/(sigma <UP><SUB><IT>z</IT></SUB><SUP><IT>2</IT></SUP></UP> sigma <UP><SUB><IT>&eegr;</IT></SUB><SUP><IT>2</IT></SUP></UP>) (25). The observed correlation |R| = 0.80 then yields sigma <UP><SUB><IT>z</IT></SUB><SUP><IT>2</IT></SUP></UP>/sigma <UP><SUB><IT>&eegr;</IT></SUB><SUP><IT>2</IT></SUP></UP> = 4, or that the rms signal fluctuation is twice that of the noise. The rms signal-to-noise ratio of zeta  can be as large as a factor of <RAD><RCD>2</RCD></RAD> greater, i.e., it should range between about 2 and 3.


    References
Top
Abstract
Introduction
Strontium and Carbon Isotopic...
Removal of the Effects...
Relationship to CO2 Levels
Estimation of the CO2...
Comparison with the Climate...
Discussion and Conclusion
References

1. Walker, J. C. G. (1977) Evolution of the Atmosphere (Macmillan, New York).
2. Holland, H. D. (1978) The Chemistry of the Atmosphere and Oceans (Wiley, New York).
3. Hayes, J. M. , Strauss, H. & Kaufman, A. J. (1999) Chem. Geol. 161, 103-125.
4. Veizer, J. , Ala, D. , Azmy, D. , Bruckschen, P. , Buhl, D. , Bruhn, F. , Carden, G. , Diener, A. , Ebneth, S. , Godderis, Y. , et al. (1999) Chem. Geol. 161, 59-88.
5. Freeman, K. & Hayes, J. M. (1992) Global Biogeochem. Cycles 6, 185-198.
6. Francois, L. M. & Walker, J. C. G. (1992) Am. J. Sci. 292, 81-135.
7. Berner, R. A. (1994) Am. J. Sci. 294, 56-91.
8. Rothman, D. H. (2001) Proc. Natl. Acad. Sci. USA 98, 4305-4310[Abstract/Free Full Text].
9. Edmond, J. (1992) Science 258, 1594-1597[Abstract/Free Full Text].
10. Richter, F. M. , Rowley, D. B. & DePaolo, D. J. (1992) Earth Planet. Sci. Lett. 109, 11-23.
11. Hayes, J. M. (1993) Marine Geol. 113, 111-125.
12. Derry, L. A. & France-Lanord, C. (1996) Earth Planet. Sci. Lett. 142, 59-74.
13. Quade, J. , Roe, L. , DeCelles, P. G. & Ojha, T. P. (1997) Science 276, 1828-1831[Abstract/Free Full Text].
14. Sharma, M. , Wasserburg, G. J. , Hofmann, A. & Chakrapani, G. J. (1999) Geochim. Cosmochim. Acta 63, 4005-4012.
15. Basu, A. R. , Jacobsen, S. B. , Poreda, R. J. , Dowling, C. B. & Aggarwal, P. K. (2001) Science 293, 1470-1473[Abstract/Free Full Text].
16. Garrels, R. M. & Mackenzie, F. T. (1971) Evolution of Sedimentary Rocks (Norton, New York).
17. Brass, G. W. (1976) Geochim. Cosmochim. Acta 40, 721-730.
18. Frakes, L. A. , Francis, J. E. & Syktus, J. I. (1992) Climate Modes of the Phanerozoic (Cambridge Univ. Press, Cambridge, U.K.).
19. Walter, M. R. , Veevers, J. J. , Calver, C. R. , Gorjan, P. & Hill, A. C. (2000) Precambrian Res. 100, 371-433.
20. Vio, R. , Strohmer, T. & Wamsteker, W. (2000) Publ. Astrono. Soc. Pac. 112, 74-90.
21. Press, W. H. , Flannery, B. P. , Teukolsky, S. A. & Vetterling, W. T. (1995) Numerical Recipes in C: The Art of Scientific Computing (Cambridge Univ. Press, Cambridge, U.K.).
22. Popp, B. N. , Laws, E. A. , Bidigare, R. R. , Dore, J. E. , Hanson, K. L. & Wakeham, S. G. (1998) Geochim. Cosmochim. Acta 62, 69-77.
23. Palmer, M. R. & Edmond, J. (1989) Earth Planet. Sci. Lett. 92, 11-26.
24. Urey, H. C. (1952) The Planets (Yale Univ. Press, New Haven, CT).
25. Feller, W. (1968) An Introduction to Probability Theory and Its Applications (Wiley, New York).
26. Budyko, M. I. , Ronov, A. B. & Yanshin, A. L. (1987) History of the Earth's Atmosphere (Springer, Berlin).
27. Ekart, D. D. , Cerling, T. E. , Montanez, I. P. & Tabor, N. J. (1999) Am. J. Sci. 299, 805-827.
28. Veizer, J. , Godderis, Y. & Francois, L. M. (2000) Nature (London) 408, 698-701.
29. Kump, L. R. (2000) Nature (London) 408, 651-652.
30. Crowley, T. J. & Berner, R. A. (2001) Science 292, 870-872[Free Full Text].
31. Wheat, C. G. , Feely, R. A. & Mottl, M. J. (1996) Geochim. Cosmochim. Acta 60, 3593-3608.
32. Harland, W. B. , Armstrong, R. , Cox, A. , Craig, L. , Smith, A. G. & Smith, D. G. (1990) A Geologic Time Scale 1989 (Cambridge Univ. Press, Cambridge, U.K.).
www.pnas.org/cgi/doi/10.1073/pnas.022055499
Add to CiteULike CiteULike   Add to Complore Complore   Add to Connotea Connotea   Add to Del.icio.us Del.icio.us   Add to Digg Digg    What's this?


This article has been cited by other articles in HighWire Press-hosted journals:


Home page
ScienceHome page
P. A. Raymond and J. J. Cole
Increase in the Export of Alkalinity from North America's Largest River
Science, July 4, 2003; 301(5629): 88 - 91.
[Abstract] [Full Text] [PDF]


Home page
Bulletin of Canadian Petroleum GeologyHome page
C. R. de Freitas
Are observed changes in the concentration of carbon dioxide in the atmosphere really dangerous?
Bulletin of Canadian Petroleum Geology, June 1, 2002; 50(2): 297 - 327.
[Abstract] [Full Text] [PDF]


This Article
Right arrow Abstract Freely available
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a colleague
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Similar articles in PubMed
Right arrow Alert me to new issues of the journal
Right arrow Add to My File Cabinet
Right arrow Download to citation manager
Right arrow Request Copyright Permission
Citing Articles
Right arrow Citing Articles via HighWire
Right arrow Citing Articles via CrossRef
Right arrow Citing Articles via ISI Web of Science (15)
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Rothman, D. H.
Right arrow Search for Related Content
PubMed
Right arrow PubMed Citation
Right arrow Articles by Rothman, D. H.
GeoRef
Right arrow GeoRef Citation
Social Bookmarking
 Add to CiteULike   Add to Complore   Add to Connotea   Add to Del.icio.us   Add to Digg  
What's this?