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contributor authorJohnson, David B.
contributor authorBeard, Kenneth V.
date accessioned2017-06-09T14:24:45Z
date available2017-06-09T14:24:45Z
date copyright1984/04/01
date issued1984
identifier issn0022-4928
identifier otherams-18807.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4154853
description abstractWhen raindrops collide, some of the kinetic energy involved in the collision will be available to initiate or sustain oscillations in the surviving drops. This paper presents results of a simple model of drop collisions that generates an estimate of the expected distribution of energies in an ensemble of colliding raindrops as a function of drop size and rain intensity. The results indicate that drop collisions can be an effective source of raindrop oscillations and that within any one rain shaft, it tends to produce a range of oscillation energies from intense to imperceptible. In every case, however, the fraction of drops oscillating and the severity of the oscillations increase with increasing drop size and rainfall intensity.
publisherAmerican Meteorological Society
titleOscillation Energies of Colliding Raindrops
typeJournal Paper
journal volume41
journal issue7
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1984)041<1235:OEOCR>2.0.CO;2
journal fristpage1235
journal lastpage1241
treeJournal of the Atmospheric Sciences:;1984:;Volume( 041 ):;issue: 007
contenttypeFulltext


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