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    The Evolution of Drop Spectra Due to Condensation, Coalescence and Breakup

    Source: Journal of the Atmospheric Sciences:;1975:;Volume( 032 ):;issue: 005::page 965
    Author:
    Young, Kenneth C.
    DOI: 10.1175/1520-0469(1975)032<0965:TEODSD>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A numerical model of warm rain processes incorporating activation of cloud condensation nuclei, drop growth by condensation and stochastic coalescence, and drop breakup is described. A collisional breakup model is compared to a spontaneous disintegration model and found not only to dominate over the spontaneous disintegration model but to produce an exponential spectrum in fair agreement with average observed drop spectra. The steady-state spectrum was found to be quite insensitive to the number of satellite drops farmed by collision or their size distribution. The effect of the finite-difference solution to the collection and breakup equations is analysed. A properly stochastic formulation for finite time steps is presented but found to differ only slightly from the simpler, ?discrete? formulation. Time stops of 5 s and 45 size categories are found adequate to describe the essential quantitative features of more intensive treatments. The model results were found to be somewhat sensitive to values used for the collection efficiency.
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      The Evolution of Drop Spectra Due to Condensation, Coalescence and Breakup

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4152643
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    contributor authorYoung, Kenneth C.
    date accessioned2017-06-09T14:18:10Z
    date available2017-06-09T14:18:10Z
    date copyright1975/05/01
    date issued1975
    identifier issn0022-4928
    identifier otherams-16818.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4152643
    description abstractA numerical model of warm rain processes incorporating activation of cloud condensation nuclei, drop growth by condensation and stochastic coalescence, and drop breakup is described. A collisional breakup model is compared to a spontaneous disintegration model and found not only to dominate over the spontaneous disintegration model but to produce an exponential spectrum in fair agreement with average observed drop spectra. The steady-state spectrum was found to be quite insensitive to the number of satellite drops farmed by collision or their size distribution. The effect of the finite-difference solution to the collection and breakup equations is analysed. A properly stochastic formulation for finite time steps is presented but found to differ only slightly from the simpler, ?discrete? formulation. Time stops of 5 s and 45 size categories are found adequate to describe the essential quantitative features of more intensive treatments. The model results were found to be somewhat sensitive to values used for the collection efficiency.
    publisherAmerican Meteorological Society
    titleThe Evolution of Drop Spectra Due to Condensation, Coalescence and Breakup
    typeJournal Paper
    journal volume32
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1975)032<0965:TEODSD>2.0.CO;2
    journal fristpage965
    journal lastpage973
    treeJournal of the Atmospheric Sciences:;1975:;Volume( 032 ):;issue: 005
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian