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    The Effects of Scattering and Ground Reflection on the Solar Energy Absorbed by Ozone in a Rayleigh Atmosphere

    Source: Journal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 002::page 175
    Author:
    Dave, J. V.
    ,
    Furukawa, P. M.
    DOI: 10.1175/1520-0469(1967)024<0175:TEOSAG>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The effects of Rayleigh scattering and Lambert ground reflection on the solar energy absorbed by ozone in the earth's molecular atmosphere are evaluated on the basis of a complete solution of the transfer equation. The results show that these processes increase the following over that for a purely-absorbing atmosphere: 1) the total solar energy absorbed by ozone in a unit atmospheric column, 2) the energy absorbed per unit mass of air at all levels (except below 100 mb at low sun), and 3) the heating rates due to the absorption of solar energy by ozone. In each case, the magnitude of the increase can vary considerably depending on the solar zenith angle and the reflectivity of the underlying surface.
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      The Effects of Scattering and Ground Reflection on the Solar Energy Absorbed by Ozone in a Rayleigh Atmosphere

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4150954
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    • Journal of the Atmospheric Sciences

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    contributor authorDave, J. V.
    contributor authorFurukawa, P. M.
    date accessioned2017-06-09T14:14:04Z
    date available2017-06-09T14:14:04Z
    date copyright1967/03/01
    date issued1967
    identifier issn0022-4928
    identifier otherams-15298.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150954
    description abstractThe effects of Rayleigh scattering and Lambert ground reflection on the solar energy absorbed by ozone in the earth's molecular atmosphere are evaluated on the basis of a complete solution of the transfer equation. The results show that these processes increase the following over that for a purely-absorbing atmosphere: 1) the total solar energy absorbed by ozone in a unit atmospheric column, 2) the energy absorbed per unit mass of air at all levels (except below 100 mb at low sun), and 3) the heating rates due to the absorption of solar energy by ozone. In each case, the magnitude of the increase can vary considerably depending on the solar zenith angle and the reflectivity of the underlying surface.
    publisherAmerican Meteorological Society
    titleThe Effects of Scattering and Ground Reflection on the Solar Energy Absorbed by Ozone in a Rayleigh Atmosphere
    typeJournal Paper
    journal volume24
    journal issue2
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1967)024<0175:TEOSAG>2.0.CO;2
    journal fristpage175
    journal lastpage181
    treeJournal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 002
    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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