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Detailed Reference Information |
Jenkins, G.S. (2001). High-obliquity simulations for the Archean Earth: Implications for climatic conditions on early Mars. Journal of Geophysical Research 106: doi: 10.1029/2000JE001427. issn: 0148-0227. |
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Global climate model simulations using high-obliquity (70¿), higher CO2 and CH4 but reduced O3 concentrations produce warm climate conditions for Archean boundary conditions (reduced solar forcing). Solar radiation under high-obliquity is distribution in such a way as to warm high latitudes and cool low-latitudes. Global mean air temperatures of approximately 280 ¿K are found with a 25% reduction in the solar forcing, 4760 ppmv CO2 and 25 ppmv CH4. High-obliquity could also explain why polar oceans on Mars may have occurred in its history. A substantial increase in the amount of insolation is accounted for if Mars had an obliquity of 70¿. ¿ 2001 American Geophysical Union |
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Abstract![](/images/icons/spacer.gif) |
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Keywords
Atmospheric Composition and Structure, Meteorology and Atmospheric Dynamics, General circulation, Meteorology and Atmospheric Dynamics, Paleoclimatology, Planetology, Solid Surface Planets, Atmospheres—composition and chemistry |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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