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contributor authorvon Storch, Jin-Song
date accessioned2017-06-09T14:37:00Z
date available2017-06-09T14:37:00Z
date copyright2001/07/01
date issued2001
identifier issn0022-4928
identifier otherams-22885.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159384
description abstractThe axial Ω and relative angular momenta, MΩ and Mr, depend on the meridional mass distribution and relative zonal velocity, respectively. According to the conventional formulation, the time rate of change of MΩ is determined by the Coriolis conversion induced by meridional velocity, C, whereas Mr is accelerated by C and the friction and pressure torques. This note decomposes C into three components, according to different ways of distributing mass in meridional direction. It is shown that the first two components are identical to the pressure and friction torque, respectively, and the last one equals the conversion induced by the ageostrophic meridional flow, Ca. The decomposition identifies Ca as the only forcing of Mr. The resulting budgets suggest that the torques change the angular momentum of a rotating fluid with the aid of mass transports, rather than by directly accelerating the rotation speed, as in the case of a rigid body.
publisherAmerican Meteorological Society
titleHow Do Friction and Pressure Torques Affect the Relative and Ω Angular Momenta of the Atmosphere?
typeJournal Paper
journal volume58
journal issue14
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(2001)058<1995:HDFAPT>2.0.CO;2
journal fristpage1995
journal lastpage1999
treeJournal of the Atmospheric Sciences:;2001:;Volume( 058 ):;issue: 014
contenttypeFulltext


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