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contributor authorFoster, Ralph C.
contributor authorLevy, Gad
date accessioned2017-06-09T14:34:59Z
date available2017-06-09T14:34:59Z
date copyright1998/04/01
date issued1998
identifier issn0022-4928
identifier otherams-22169.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4158589
description abstractObservations show that, for a given geostrophic forcing, baroclinity acting on the planetary boundary layer produces a nearly sinusoidal modification of the near-surface wind. Compared to barotropic conditions the speed is enhanced in the direction of the thermal wind and the cross-isobar angle increases (decreases) in cold (warm) advection. These modifications are asymmetric with respect to the thermal wind orientation. Two-layer similarity models that match a stratification-dependent surface layer to a stratification and baroclinity dependent Ekman layer simulate aspects of this asymmetric baroclinic modification if the cold advection conditions are more unstably stratified than the warm advection conditions. The authors demonstrate that roll vortices in a baroclinic planetary boundary layer produce an asymmetric surface wind modification in neutral stratification that can work in concert with the coupling between stratification and baroclinity to enhance the net effect of baroclinity on the surface wind. It is further demonstrated that the roll modification effect can be as much as or even more that the pure thermal wind effect, although both are secondary to the pure frictional effect. This baroclinic roll modification works to increase the low-level poleward mass transport and the near-surface westerly momentum in the midlatitudes.
publisherAmerican Meteorological Society
titleThe Contribution of Organized Roll Vortices to the Surface Wind Vector in Baroclinic Conditions
typeJournal Paper
journal volume55
journal issue8
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1998)055<1466:TCOORV>2.0.CO;2
journal fristpage1466
journal lastpage1472
treeJournal of the Atmospheric Sciences:;1998:;Volume( 055 ):;issue: 008
contenttypeFulltext


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