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    Fluctuation Properties of Precipitation. Part V: Distribution of Rain Rates—Theory and Observations in Clustered Rain

    Source: Journal of the Atmospheric Sciences:;1999:;Volume( 056 ):;issue: 022::page 3920
    Author:
    Jameson, A. R.
    ,
    Kostinski, A. B.
    DOI: 10.1175/1520-0469(1999)056<3920:FPOPPV>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Recent studies have led to the statistical characterization of the flux of drops of a particular size as a doubly stochastic Poisson process (Poisson mixture). Moreover, previous papers in this series show that the fluxes at different sizes are correlated among each other both temporally and spatially over many different scales. Thus, in general, rather than being distributed evenly, significant clustering or bunching of the rain occurs. That is, regions richer in drops are interspersed with those where drops are scarcer. This work applies these recent findings to explore the statistical characteristics of the rainfall rate itself, a triply stochastic random variable resulting from the summation over all the fluxes at different drop sizes. Among the findings, it is shown that clustering of the drops leads to increased frequencies of both smaller and larger rainfall rates. That is, because of clustering, drop rich regions boost the frequency of large rainfall rates, while the likelihood of light rainfall rates increases because of drop poor regions. These results, derived using detailed, physically based Monte Carlo simulations of clustered rain, agree with video-disdrometer observations. Moreover, it is shown that for a given mean rainfall rate, extensive averaging lengthens the tail of the probability density function (pdf) of the rainfall rate, P(R). While the tail of the P(R) for clustered rain is sometimes reminiscent of that of the oft-used lognormal distribution, it is shown that the lognormal pdf is a poor match to the observations and simulations. It is concluded that the lognormal distribution is inconsistent with the statistical physics of natural, clustered rain. It is also argued that for clustered rain, the relative dispersion of the rainfall rate is proportional to the relative dispersion in the total number of drops in the volumes sampled. While the constant of proportionality depends upon drop diameter, observations demonstrate that the relative dispersion in the rainfall rate is due much more to the variability in the number of drops in the sampled volumes than to variations in drop sizes. The results in this work are likely relevant to such areas of research as remote sensing and hydrology.
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      Fluctuation Properties of Precipitation. Part V: Distribution of Rain Rates—Theory and Observations in Clustered Rain

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4158946
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    contributor authorJameson, A. R.
    contributor authorKostinski, A. B.
    date accessioned2017-06-09T14:35:51Z
    date available2017-06-09T14:35:51Z
    date copyright1999/11/01
    date issued1999
    identifier issn0022-4928
    identifier otherams-22490.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4158946
    description abstractRecent studies have led to the statistical characterization of the flux of drops of a particular size as a doubly stochastic Poisson process (Poisson mixture). Moreover, previous papers in this series show that the fluxes at different sizes are correlated among each other both temporally and spatially over many different scales. Thus, in general, rather than being distributed evenly, significant clustering or bunching of the rain occurs. That is, regions richer in drops are interspersed with those where drops are scarcer. This work applies these recent findings to explore the statistical characteristics of the rainfall rate itself, a triply stochastic random variable resulting from the summation over all the fluxes at different drop sizes. Among the findings, it is shown that clustering of the drops leads to increased frequencies of both smaller and larger rainfall rates. That is, because of clustering, drop rich regions boost the frequency of large rainfall rates, while the likelihood of light rainfall rates increases because of drop poor regions. These results, derived using detailed, physically based Monte Carlo simulations of clustered rain, agree with video-disdrometer observations. Moreover, it is shown that for a given mean rainfall rate, extensive averaging lengthens the tail of the probability density function (pdf) of the rainfall rate, P(R). While the tail of the P(R) for clustered rain is sometimes reminiscent of that of the oft-used lognormal distribution, it is shown that the lognormal pdf is a poor match to the observations and simulations. It is concluded that the lognormal distribution is inconsistent with the statistical physics of natural, clustered rain. It is also argued that for clustered rain, the relative dispersion of the rainfall rate is proportional to the relative dispersion in the total number of drops in the volumes sampled. While the constant of proportionality depends upon drop diameter, observations demonstrate that the relative dispersion in the rainfall rate is due much more to the variability in the number of drops in the sampled volumes than to variations in drop sizes. The results in this work are likely relevant to such areas of research as remote sensing and hydrology.
    publisherAmerican Meteorological Society
    titleFluctuation Properties of Precipitation. Part V: Distribution of Rain Rates—Theory and Observations in Clustered Rain
    typeJournal Paper
    journal volume56
    journal issue22
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1999)056<3920:FPOPPV>2.0.CO;2
    journal fristpage3920
    journal lastpage3932
    treeJournal of the Atmospheric Sciences:;1999:;Volume( 056 ):;issue: 022
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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