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    The Runaway Greenhouse: A History of Water on Venus

    Source: Journal of the Atmospheric Sciences:;1969:;Volume( 026 ):;issue: 006::page 1191
    Author:
    Ingersoll, Andrew P.
    DOI: 10.1175/1520-0469(1969)026<1191:TRGAHO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Radiative-convective equilibrium models of planetary atmospheres are discussed for the case when the infrared opacity is due to a vapor in equilibrium with its liquid or solid phase. For a grey gas, or for a gas which absorbs at all infrared wavelengths, equilibrium is impossible when the solar constant exceeds a critical value. Equilibrium therefore requires that the condensed phase evaporates into the atmosphere. Moist adiabatic and pseudoadiabatic atmospheres in which the condensing vapor is a major atmospheric constituent are considered. This situation would apply if the solar constant were supercritical with respect to an abundant substance such as water. It is shown that the condensing gas would be a major constituent at all levels in such an atmosphere. Photodissociation of water in the primordial Venus atmosphere is discussed in this context.
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      The Runaway Greenhouse: A History of Water on Venus

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4151406
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    contributor authorIngersoll, Andrew P.
    date accessioned2017-06-09T14:15:09Z
    date available2017-06-09T14:15:09Z
    date copyright1969/11/01
    date issued1969
    identifier issn0022-4928
    identifier otherams-15704.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151406
    description abstractRadiative-convective equilibrium models of planetary atmospheres are discussed for the case when the infrared opacity is due to a vapor in equilibrium with its liquid or solid phase. For a grey gas, or for a gas which absorbs at all infrared wavelengths, equilibrium is impossible when the solar constant exceeds a critical value. Equilibrium therefore requires that the condensed phase evaporates into the atmosphere. Moist adiabatic and pseudoadiabatic atmospheres in which the condensing vapor is a major atmospheric constituent are considered. This situation would apply if the solar constant were supercritical with respect to an abundant substance such as water. It is shown that the condensing gas would be a major constituent at all levels in such an atmosphere. Photodissociation of water in the primordial Venus atmosphere is discussed in this context.
    publisherAmerican Meteorological Society
    titleThe Runaway Greenhouse: A History of Water on Venus
    typeJournal Paper
    journal volume26
    journal issue6
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1969)026<1191:TRGAHO>2.0.CO;2
    journal fristpage1191
    journal lastpage1198
    treeJournal of the Atmospheric Sciences:;1969:;Volume( 026 ):;issue: 006
    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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