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    A Numerical Solution to the Equation of Radiative Transfer

    Source: Journal of the Atmospheric Sciences:;1965:;Volume( 022 ):;issue: 005::page 559
    Author:
    Herman, Benjamin M.
    ,
    Browning, Samuel R.
    DOI: 10.1175/1520-0469(1965)022<0559:ANSTTE>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A numerical method of solving the equation of radiative transfer for a plane parallel, horizontally homogeneous medium is presented. The method is applicable for problems with nonconservative scattering as well as for conservative scattering problems. Comparison of results for the reflected and transmitted radiation from this method with existing solutions for conservative Rayleigh scattering shows that, for optical depths up to 1-0, the present scheme is accurate to within ±0.007 unit total intensity and ±1.0 per cent polarization for an incident flux of π units per unit normal area. Results are presented for the reflected and transmitted intensity and per cent polarization for optical depths 2.0 and 4.0, for a particular problem of conservative Rayleigh scattering.
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      A Numerical Solution to the Equation of Radiative Transfer

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4150771
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    • Journal of the Atmospheric Sciences

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    contributor authorHerman, Benjamin M.
    contributor authorBrowning, Samuel R.
    date accessioned2017-06-09T14:13:37Z
    date available2017-06-09T14:13:37Z
    date copyright1965/09/01
    date issued1965
    identifier issn0022-4928
    identifier otherams-15132.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150771
    description abstractA numerical method of solving the equation of radiative transfer for a plane parallel, horizontally homogeneous medium is presented. The method is applicable for problems with nonconservative scattering as well as for conservative scattering problems. Comparison of results for the reflected and transmitted radiation from this method with existing solutions for conservative Rayleigh scattering shows that, for optical depths up to 1-0, the present scheme is accurate to within ±0.007 unit total intensity and ±1.0 per cent polarization for an incident flux of π units per unit normal area. Results are presented for the reflected and transmitted intensity and per cent polarization for optical depths 2.0 and 4.0, for a particular problem of conservative Rayleigh scattering.
    publisherAmerican Meteorological Society
    titleA Numerical Solution to the Equation of Radiative Transfer
    typeJournal Paper
    journal volume22
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1965)022<0559:ANSTTE>2.0.CO;2
    journal fristpage559
    journal lastpage566
    treeJournal of the Atmospheric Sciences:;1965:;Volume( 022 ):;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