YaBeSH Engineering and Technology Library

    • Journals
    • PaperQuest
    • YSE Standards
    • YaBeSH
    • Login
    View Item 
    •   YE&T Library
    • AMS
    • Journal of the Atmospheric Sciences
    • View Item
    •   YE&T Library
    • AMS
    • Journal of the Atmospheric Sciences
    • View Item
    • All Fields
    • Source Title
    • Year
    • Publisher
    • Title
    • Subject
    • Author
    • DOI
    • ISBN
    Advanced Search
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Archive

    On the Fractional Scattering into the Forward Peak

    Source: Journal of the Atmospheric Sciences:;1999:;Volume( 056 ):;issue: 015::page 2728
    Author:
    Li, J.
    DOI: 10.1175/1520-0469(1999)056<2728:OTFSIT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A hypothesis that the fractional scattering into the forward peak is related to solar zenith angle and single scattering albedo is proposed. Calculations show that this assumption can increase the accuracy of the δ-Eddington approximation. For the scattering conservative case this method can improve the results in the region of thin optical depth. For the scattering nonconservative case this method can reduce the errors for reflection and absorption in the region of small solar zenith angle, where the incoming solar energy is most significant.
    • Download: (984.9Kb)
    • Show Full MetaData Hide Full MetaData
    • Item Order
    • Go To Publisher
    • Price: 5000 Rial
    • Statistics

      On the Fractional Scattering into the Forward Peak

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4158861
    Collections
    • Journal of the Atmospheric Sciences

    Show full item record

    contributor authorLi, J.
    date accessioned2017-06-09T14:35:38Z
    date available2017-06-09T14:35:38Z
    date copyright1999/08/01
    date issued1999
    identifier issn0022-4928
    identifier otherams-22413.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4158861
    description abstractA hypothesis that the fractional scattering into the forward peak is related to solar zenith angle and single scattering albedo is proposed. Calculations show that this assumption can increase the accuracy of the δ-Eddington approximation. For the scattering conservative case this method can improve the results in the region of thin optical depth. For the scattering nonconservative case this method can reduce the errors for reflection and absorption in the region of small solar zenith angle, where the incoming solar energy is most significant.
    publisherAmerican Meteorological Society
    titleOn the Fractional Scattering into the Forward Peak
    typeJournal Paper
    journal volume56
    journal issue15
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1999)056<2728:OTFSIT>2.0.CO;2
    journal fristpage2728
    journal lastpage2732
    treeJournal of the Atmospheric Sciences:;1999:;Volume( 056 ):;issue: 015
    contenttypeFulltext
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian
     
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian