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    An Analytical and Numerical Study of the Martian Planetary Boundary Layer Over Slopes

    Source: Journal of the Atmospheric Sciences:;1973:;Volume( 030 ):;issue: 001::page 66
    Author:
    Blumsack, Steven L.
    ,
    Gierasch, Peter J.
    ,
    Wessel, W. Roy
    DOI: 10.1175/1520-0469(1973)030<0066:AAANSO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A one-dimensional model of the Martian planetary boundary layer over sloping terrain is analyzed under a variety of conditions. Analytical results for the steady and diurnal components of the temperature and wind fields are found when a Boussinesq model with a Newtonian cooling law is considered. These results form a basis for understanding the numerical results which include more realistic representations for the heating and parameterizations for the eddy transfer of momentum and beat. The diurnal boundary layer thickness is determined primarily by radiative processes and the amplitudes of the wind and temperature oscillations are found to depend in an important way on the latitude and slope magnitude. Typically, oscillations in the temperature of ±15K and in the upslope wind of ±25m sec ?1 are found 1 km above a Martian slope of 0.005.
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      An Analytical and Numerical Study of the Martian Planetary Boundary Layer Over Slopes

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4152063
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    • Journal of the Atmospheric Sciences

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    contributor authorBlumsack, Steven L.
    contributor authorGierasch, Peter J.
    contributor authorWessel, W. Roy
    date accessioned2017-06-09T14:16:44Z
    date available2017-06-09T14:16:44Z
    date copyright1973/01/01
    date issued1973
    identifier issn0022-4928
    identifier otherams-16296.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4152063
    description abstractA one-dimensional model of the Martian planetary boundary layer over sloping terrain is analyzed under a variety of conditions. Analytical results for the steady and diurnal components of the temperature and wind fields are found when a Boussinesq model with a Newtonian cooling law is considered. These results form a basis for understanding the numerical results which include more realistic representations for the heating and parameterizations for the eddy transfer of momentum and beat. The diurnal boundary layer thickness is determined primarily by radiative processes and the amplitudes of the wind and temperature oscillations are found to depend in an important way on the latitude and slope magnitude. Typically, oscillations in the temperature of ±15K and in the upslope wind of ±25m sec ?1 are found 1 km above a Martian slope of 0.005.
    publisherAmerican Meteorological Society
    titleAn Analytical and Numerical Study of the Martian Planetary Boundary Layer Over Slopes
    typeJournal Paper
    journal volume30
    journal issue1
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1973)030<0066:AAANSO>2.0.CO;2
    journal fristpage66
    journal lastpage82
    treeJournal of the Atmospheric Sciences:;1973:;Volume( 030 ):;issue: 001
    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