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contributor authorHyun, Jae Min
contributor authorPeskin, Richard L.
date accessioned2017-06-09T14:19:57Z
date available2017-06-09T14:19:57Z
date copyright1978/02/01
date issued1978
identifier issn0022-4928
identifier otherams-17421.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153314
description abstractNumerical computations are conducted to investigate the deep-fluid effects on the baroclinically unstable waves whose nondimensional wavenumbers are of order unity[k?O(1),llsim;(1)]. Two representative values of the Richardson number, Ri=0.5 and Ri=2.0, are used in the actual computations. The mass-divergence effect appears to reduce principally the propagation speed and, to a degree, the growth rate in both instability regimes. In particular, the mass-divergence effect affects the wave structure of the vertical velocity, shifting the vertical level of Wmax. Also, the latitudinal wavenumber dependence of the eigenvalue is examined.
publisherAmerican Meteorological Society
titleBaroclinic Instabilities of A Deep Fluid. Part II
typeJournal Paper
journal volume35
journal issue2
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1978)035<0169:BIOADF>2.0.CO;2
journal fristpage169
journal lastpage174
treeJournal of the Atmospheric Sciences:;1978:;Volume( 035 ):;issue: 002
contenttypeFulltext


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