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14 - Carbon dioxide and Phanerozoic climate

from Part V - Overview: climate across tectonic timescales

Published online by Cambridge University Press:  06 July 2010

Brian T. Huber
Affiliation:
Smithsonian Institution, Washington DC
Kenneth G. Macleod
Affiliation:
University of Missouri, Columbia
Scott L. Wing
Affiliation:
Smithsonian Institution, Washington DC
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Summary

ABSTRACT

Much has been written about the importance of past carbon dioxide fluctuations as a cause of Phanerozoic climate change. In this update I summarize the present level of data/CO2 geochemical model agreement for the Phanerozoic. Although there is a striking first-order agreement between simulated changes in CO2, proxy estimates of CO2, and evidence for global climate change, I argue that additional factors need to be considered in order to derive a general theory for Phanerozoic climates that is in quantitative agreement with climate models, and that these factors fall into two levels of importance. The most important first-order considerations for global temperature involve land–sea distribution and solar luminosity changes. Changes in ocean heat transport, orography, and vegetation may be necessary for obtaining better agreement between spatial patterns of climate change and models, but they may have a second-order effect on global temperature except in some cases of high latitude vegetation cover and the effect of orography on CO2 levels. A more complete explanation for climate on tectonic time scales has to incorporate all these factors in a parsimonious manner in order to avoid a proliferation of ad hoc explanations for past climate change. Enhanced statistical comparisons between models and data are essential for more stringent testing of model predictions.

INTRODUCTION

Since the groundbreaking work of Eric Barron, Robert Berner and colleagues in the early 1980s much has been learned about causes of climate change on tectonic time scales.

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Publisher: Cambridge University Press
Print publication year: 1999

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