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    ON THE RADIATIVE EQUILIBRIUM AND HEAT BALANCE OF THE ATMOSPHERE

    Source: Monthly Weather Review:;1961:;volume( 089 ):;issue: 012::page 503
    Author:
    MANABE, SYUKURO
    ,
    MÖLLER, FRITZ
    DOI: 10.1175/1520-0493(1961)089<0503:OTREAH>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: In order to incorporate the effect of radiation into the numerical experiment of the general circulation of the atmosphere, a simplified scheme for computing the radiative temperature change is constructed. The effects included are long wave radiation by water vapor, carbon dioxide, and ozone and the absorption of solar radiation by these three gases. The absorptivities of these gases are determined based upon the recent results of laboratory experiments and those of theoretical computations. The effects of clouds are not included. By use of this scheme the radiative equilibrium temperature is computed for various latitudes and seasons as asymptotic solutions of an initial value problem. To a certain degree the radiative equilibrium solutions reveal some of the typical characteristics of stratospheric temperature and tropopause height variations. Radiative heat budgets of the atmosphere are also computed and compared with the results of the computations of radiative equilibrium. This comparison is helpful for understanding the role of radiative processes and also suggests the kinds of effect we should expect from other thermal processes in the atmosphere.
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      ON THE RADIATIVE EQUILIBRIUM AND HEAT BALANCE OF THE ATMOSPHERE

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4197571
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    • Monthly Weather Review

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    contributor authorMANABE, SYUKURO
    contributor authorMÖLLER, FRITZ
    date accessioned2017-06-09T15:56:57Z
    date available2017-06-09T15:56:57Z
    date copyright1961/12/01
    date issued1961
    identifier issn0027-0644
    identifier otherams-57255.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4197571
    description abstractIn order to incorporate the effect of radiation into the numerical experiment of the general circulation of the atmosphere, a simplified scheme for computing the radiative temperature change is constructed. The effects included are long wave radiation by water vapor, carbon dioxide, and ozone and the absorption of solar radiation by these three gases. The absorptivities of these gases are determined based upon the recent results of laboratory experiments and those of theoretical computations. The effects of clouds are not included. By use of this scheme the radiative equilibrium temperature is computed for various latitudes and seasons as asymptotic solutions of an initial value problem. To a certain degree the radiative equilibrium solutions reveal some of the typical characteristics of stratospheric temperature and tropopause height variations. Radiative heat budgets of the atmosphere are also computed and compared with the results of the computations of radiative equilibrium. This comparison is helpful for understanding the role of radiative processes and also suggests the kinds of effect we should expect from other thermal processes in the atmosphere.
    publisherAmerican Meteorological Society
    titleON THE RADIATIVE EQUILIBRIUM AND HEAT BALANCE OF THE ATMOSPHERE
    typeJournal Paper
    journal volume89
    journal issue12
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1961)089<0503:OTREAH>2.0.CO;2
    journal fristpage503
    journal lastpage532
    treeMonthly Weather Review:;1961:;volume( 089 ):;issue: 012
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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