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contributor authorWebb, Willis L.
date accessioned2017-06-09T14:13:53Z
date available2017-06-09T14:13:53Z
date copyright1966/09/01
date issued1966
identifier issn0022-4928
identifier otherams-15233.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150883
description abstractRotation of the earth introduces a diurnal perturbation into the heating experienced by the ozonosphere through absorption of solar ultraviolet radiant energy. This diurnal heat wave induces perturbations in the stratospheric wind field which are principally meridional at low latitudes and are largely zonal at high latitudes. This asymmetric situation is shown to power a tidal-type circulation system which has its maximum strength in the high latitude nighttime upper mesosphere of the summer hemisphere. This ?stratospheric tidal jet? is zonal as it skirts the periphery of the continuously heated polar region, and presumably serves to transport and mix the summer mesosphere as well as provide the vertical flow required for formation of noctilucent clouds.
publisherAmerican Meteorological Society
titleThe Stratospheric Tidal Jet
typeJournal Paper
journal volume23
journal issue5
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1966)023<0531:TSTJ>2.0.CO;2
journal fristpage531
journal lastpage534
treeJournal of the Atmospheric Sciences:;1966:;Volume( 023 ):;issue: 005
contenttypeFulltext


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