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    KINEMATICAL RELATIONS BETWEEN WIND AND PRECIPITATION DISTRIBUTIONS

    Source: Journal of Meteorology:;1959:;volume( 016 ):;issue: 006::page 630
    Author:
    Kessler, Edwin
    DOI: 10.1175/1520-0469(1959)016<0630:KRBWAP>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: If distributions of precipitation in the atmosphere could be understood in terms of their associated three-dimensional winds, then radar, radiosonde, and surface observations might be utilized in new ways as sources of information about the winds. In this paper, continuity equations for precipitation content of horizontally uniform updrafts, or to the cores of simple cells such as represented by showers formed in the absence of vertical wind shear. A parabolic profile of updrafts is assumed. When the precipitation profile is steady-state and the fall speed of precipitation is constant, the amount of precipitation per unit volume of air increases rapidly downward in mid-atmosphere. Near the surface, changes in the vertical are very small. Maxima of precipitation content occur aloft before steady conditions obtain throughout the updraft layer; in the steady case, maxima aloft may occur when the terminal fall speed of precipitation increases only slightly faster than the updrafts and with little increase of fall speed during their growth, as is often the case with snow. An explanation is offered for the difference between the vertical distributions of precipitation associated with widespread systems and with showers, and means for practical utilization of the results are suggested.
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      KINEMATICAL RELATIONS BETWEEN WIND AND PRECIPITATION DISTRIBUTIONS

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4150150
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    contributor authorKessler, Edwin
    date accessioned2017-06-09T14:12:14Z
    date available2017-06-09T14:12:14Z
    date copyright1959/12/01
    date issued1959
    identifier issn0095-9634
    identifier otherams-14574.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150150
    description abstractIf distributions of precipitation in the atmosphere could be understood in terms of their associated three-dimensional winds, then radar, radiosonde, and surface observations might be utilized in new ways as sources of information about the winds. In this paper, continuity equations for precipitation content of horizontally uniform updrafts, or to the cores of simple cells such as represented by showers formed in the absence of vertical wind shear. A parabolic profile of updrafts is assumed. When the precipitation profile is steady-state and the fall speed of precipitation is constant, the amount of precipitation per unit volume of air increases rapidly downward in mid-atmosphere. Near the surface, changes in the vertical are very small. Maxima of precipitation content occur aloft before steady conditions obtain throughout the updraft layer; in the steady case, maxima aloft may occur when the terminal fall speed of precipitation increases only slightly faster than the updrafts and with little increase of fall speed during their growth, as is often the case with snow. An explanation is offered for the difference between the vertical distributions of precipitation associated with widespread systems and with showers, and means for practical utilization of the results are suggested.
    publisherAmerican Meteorological Society
    titleKINEMATICAL RELATIONS BETWEEN WIND AND PRECIPITATION DISTRIBUTIONS
    typeJournal Paper
    journal volume16
    journal issue6
    journal titleJournal of Meteorology
    identifier doi10.1175/1520-0469(1959)016<0630:KRBWAP>2.0.CO;2
    journal fristpage630
    journal lastpage637
    treeJournal of Meteorology:;1959:;volume( 016 ):;issue: 006
    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
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