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contributor authorArya, S. P. S.
date accessioned2017-06-09T14:19:55Z
date available2017-06-09T14:19:55Z
date copyright1978/01/01
date issued1978
identifier issn0022-4928
identifier otherams-17409.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153300
description abstractThe effects of baroclinity and the scale-height ratio on the drag laws of the planetary boundary layer (PBL) are examined theoretically and compared to those of stability. The similarity drag relations using surface geostrophic winds are found to be more sensitive to these parameters than the drag relations based on the layer-averaged winds. Since baroclinity can be more safely ignored in the latter, these are considered more suitable for parameterizing the PBL in general circulation models. The geostrophic drag relations based on the generalized similarity theory are used to explain (simulate) the observed increasing trend of the surface cross-isobar angle in going toward the equator. It is shown that this trend is partly due to the change in the scale-height ratio and partly due to baroclinity. Clarke and Mess (1975), on the other hand, have suggested that baroclinity is wholly responsible for this trend. It is shown here that baroclinity effects are very much exaggerated in their formulation.
publisherAmerican Meteorological Society
titleComparative Effects of Stability, Baroclinity and the Scale-Height Ratio on Drag Laws for the Atmospheric Boundary Layer
typeJournal Paper
journal volume35
journal issue1
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1978)035<0040:CEOSBA>2.0.CO;2
journal fristpage40
journal lastpage46
treeJournal of the Atmospheric Sciences:;1978:;Volume( 035 ):;issue: 001
contenttypeFulltext


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