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contributor authorPierrehumbert, R. T.
contributor authorErlick, C.
date accessioned2017-06-09T14:35:04Z
date available2017-06-09T14:35:04Z
date copyright1998/05/01
date issued1998
identifier issn0022-4928
identifier otherams-22192.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4158615
description abstractThe authors offer some remarks on the greenhouse effect due to high clouds that reflect thermal infrared radiation, but do not absorb or emit it. Such clouds are an idealization of the CO2 ice clouds that are thought to have existed early in the history of Mars. Clouds of this type enter also in the ability of Earth to recover from a globally glaciated ?cold start? and in the determination of habitable zones of planetary systems. A simplified model of cloud optical effects is used to estimate the effect of high CO2 ice clouds on the planetary radiation budget in the solar and infrared spectrum. It is argued that the scattering greenhouse effect certainly cancels out a large part of the cooling effect due to the cloud?s visible albedo and in some circumstances may even lead to a net warming as compared to the no-cloud case. Speculative implications for the climate of early Mars are discussed.
publisherAmerican Meteorological Society
titleOn the Scattering Greenhouse Effect of CO2 Ice Clouds
typeJournal Paper
journal volume55
journal issue10
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1998)055<1897:OTSGEO>2.0.CO;2
journal fristpage1897
journal lastpage1903
treeJournal of the Atmospheric Sciences:;1998:;Volume( 055 ):;issue: 010
contenttypeFulltext


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