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contributor authorRyzhkov, Alexander V.
contributor authorZrnić, Dusan S.
date accessioned2017-06-09T14:34:08Z
date available2017-06-09T14:34:08Z
date copyright1996/10/01
date issued1996
identifier issn0022-4928
identifier otherams-21856.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4158241
description abstractThe authors contrast rainfall in two Oklahoma squall lines: one with deep convection occurred in the spring and the other with shallower convection in the winter. Both passed over a micronetwork of densely spaced rain gauges and were observed with the National Severe Storm Laboratory's polarimetric weather radar. Polarimetric measurements reveal differences in storm structure that in turn imply that microphysical processes caused the drop size distributions to be quite distinct for the two events. In the winter squall line the conventional R(Z) algorithm for estimating rainfall fails badly, whereas in the summer squall line it performs well. The method based on specific differential phase measurements, however, yields a very good match between radar-derived areal precipitation amount and rain depth obtained from the micronetwork of densely located rain gauges for both events.
publisherAmerican Meteorological Society
titleRain in Shallow and Deep Convection Measured with a Polarimetric Radar
typeJournal Paper
journal volume53
journal issue20
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1996)053<2989:RISADC>2.0.CO;2
journal fristpage2989
journal lastpage2995
treeJournal of the Atmospheric Sciences:;1996:;Volume( 053 ):;issue: 020
contenttypeFulltext


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