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contributor authorHou, Arthur Y.
contributor authorFels, Stephen B.
contributor authorGoody, Richard M.
date accessioned2017-06-09T14:29:51Z
date available2017-06-09T14:29:51Z
date copyright1990/08/01
date issued1989
identifier issn0022-4928
identifier otherams-20366.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156586
description abstractWe have calculated the equilibrium zonal wind structure resulting from the interaction of the semidiurnal tide and the mean meridional circulation driven by the zonally averaged solar heating above the Venus cloud base. The results show that the tidal mechanism proposed by Fels and Lindzen can account for a substantial fraction?and possibly all?of the increase of the equatorial wind speed above the cloud base. Above the cloud tops, tidal deceleration may be too small to produce the zonal wind decrease with height inferred from thermal data. Tidal forcing does not explain the superrotation below the clouds and additional eddy sources are needed to account for the zonal wind structure at mid and high latitudes.
publisherAmerican Meteorological Society
titleZonal Superrotation above Venus' Cloud Base Induced by the Semidiurnal Tide and the Mean Meridional Circulation
typeJournal Paper
journal volume47
journal issue15
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1990)047<1894:ZSAVCB>2.0.CO;2
journal fristpage1894
journal lastpage1901
treeJournal of the Atmospheric Sciences:;1989:;Volume( 047 ):;issue: 015
contenttypeFulltext


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