EarthRef.org Reference Database (ERR)
Development and Maintenance by the EarthRef.org Database Team

Detailed Reference Information
Jenkins 2001
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.

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

BACKGROUND DATA FILES

Abstract

Keywords
Atmospheric Composition and Structure, Meteorology and Atmospheric Dynamics, General circulation, Meteorology and Atmospheric Dynamics, Paleoclimatology, Planetology, Solid Surface Planets, Atmospheres—composition and chemistry
Journal
Journal of Geophysical Research
http://www.agu.org/journals/jb/
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
Click to clear formClick to return to previous pageClick to submit