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contributor authorKaspi, Yohai
contributor authorSchneider, Tapio
date accessioned2017-06-09T16:54:07Z
date available2017-06-09T16:54:07Z
date copyright2011/10/01
date issued2011
identifier issn0022-4928
identifier otherams-76236.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4218661
description abstracthe Northern Hemisphere storm tracks have maximum intensity over the Pacific and Atlantic basins; their intensity is reduced over the continents downstream. Here, simulations with an idealized aquaplanet general circulation model are used to demonstrate that even without continents, storm tracks have a self-determined longitudinal length scale. Their length is controlled primarily by the planetary rotation rate and is similar to that of Earth?s storm tracks for Earth?s rotation rate. Downstream, storm tracks self-destruct: the downstream eddy kinetic energy is lower than it would be without the zonal asymmetries that cause localized storm tracks. Likely involved in the downstream self-destruction of storm tracks are the energy fluxes associated with them. The zonal asymmetries that cause localized storm tracks enhance the energy transport through the generation of stationary eddies, and this leads to a reduced baroclinicity that persists far downstream of the eddy kinetic energy maxima.
publisherAmerican Meteorological Society
titleDownstream Self-Destruction of Storm Tracks
typeJournal Paper
journal volume68
journal issue10
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/JAS-D-10-05002.1
journal fristpage2459
journal lastpage2464
treeJournal of the Atmospheric Sciences:;2011:;Volume( 068 ):;issue: 010
contenttypeFulltext


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