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contributor authorGossard, E. E.
contributor authorJensen, D. R.
contributor authorRichter, S. H.
date accessioned2017-06-09T14:15:54Z
date available2017-06-09T14:15:54Z
date copyright1971/07/01
date issued1971
identifier issn0022-4928
identifier otherams-15988.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151720
description abstractIn the present paper, atmospheric structure revealed by a high-resolution FM/CW radar sounder is compared with hypothetical models of internal wave structure and convection. Special attention is given to the distribution of Richardson's number in trapped and untrapped gravity waves. It is concluded that the multiple layers result from untrapped internal gravity waves, whose propagation vector is directed newly vertically, within very stable height regions. In contrast to the convective instability proposed by Orlanski and Bryan, it is concluded that the layers are caused by Kelvin-Helmholtz instability resulting from the reduction in the Richardson's number due to growth of the amplitude-to-wavelength ratio as the waves propagate into thermally stable height regions of the atmosphere.
publisherAmerican Meteorological Society
titleAn Analytical Study of Tropospheric Structure as Seen by High-Resolution Radar
typeJournal Paper
journal volume28
journal issue5
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1971)028<0794:AASOTS>2.0.CO;2
journal fristpage794
journal lastpage807
treeJournal of the Atmospheric Sciences:;1971:;Volume( 028 ):;issue: 005
contenttypeFulltext


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