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contributor authorBalakrishnan, N.
contributor authorZrnic, D. S.
date accessioned2017-06-09T14:29:46Z
date available2017-06-09T14:29:46Z
date copyright1990/07/01
date issued1989
identifier issn0022-4928
identifier otherams-20340.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156558
description abstractWe examine the utility of the correlation coefficient between linear orthogonally polarized echoes for determining precipitation type and gauging hail size. Models and measurements from pure rain coincide in predicting very high correlations (0.98); similar results are obtained with pure hail. Several mechanisms could cause the lowering of correlation but the behavior of the examined data is definitely attributed to a mixture of hydrometeor types. This decrease is an indicator of hail size; it is shown theoretically that in at least two other realistic situations the correlation would decrease with hail size. For the examined case a model of hail shape and orientation during fall is able to reproduce the essential features of polarimetric measurements. It suggests, together with our data and data from other investigators, that substantial negative differential reflectivity (about ?1 dB) in a region of high reflectivity factor values is caused by hailstones larger than about 2 cm in diameter.
publisherAmerican Meteorological Society
titleUse of Polarization to Characterize Precipitation and Discriminate Large Hail
typeJournal Paper
journal volume47
journal issue13
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1990)047<1525:UOPTCP>2.0.CO;2
journal fristpage1525
journal lastpage1540
treeJournal of the Atmospheric Sciences:;1989:;Volume( 047 ):;issue: 013
contenttypeFulltext


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