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    Acoustic Wave Propagation in a Non-Gray Radiating Atmosphere

    Source: Journal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 005::page 808
    Author:
    Gille, John C.
    DOI: 10.1175/1520-0469(1968)025<0808:AWPIAN>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: An analysis based on radiative decay times allows the quantitative calculation of the effects of thermal radiation on acoustic wave propagation in an infinite non-gray atmosphere. Computations for the earth's troposphere, Mars, Venus, and ammonia in the laboratory show that in no case is measurable alteration of the propagation velocity predicted, but radiation is the main damping mechanism at low frequencies. Calculated damping is consistent with atmospheric observations. Laboratory demonstration of this effect is probably not possible in air, but appears feasible in low pressure ammonia. Acoustic wave propagation at high altitudes (low pressures) is shown to be adiabatic, contrary to a suggestion by Golitsyn. An approximate treatment to include the effects of the finite depth of the atmosphere shows that the results are somewhat altered in detail. An important finding is that for this problem a non-gray atmosphere cannot be usefully approximated by one or more gray coefficients. A simple approximation to the effective absorption coefficient is suggested.
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      Acoustic Wave Propagation in a Non-Gray Radiating Atmosphere

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4151169
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    contributor authorGille, John C.
    date accessioned2017-06-09T14:14:36Z
    date available2017-06-09T14:14:36Z
    date copyright1968/09/01
    date issued1968
    identifier issn0022-4928
    identifier otherams-15491.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151169
    description abstractAn analysis based on radiative decay times allows the quantitative calculation of the effects of thermal radiation on acoustic wave propagation in an infinite non-gray atmosphere. Computations for the earth's troposphere, Mars, Venus, and ammonia in the laboratory show that in no case is measurable alteration of the propagation velocity predicted, but radiation is the main damping mechanism at low frequencies. Calculated damping is consistent with atmospheric observations. Laboratory demonstration of this effect is probably not possible in air, but appears feasible in low pressure ammonia. Acoustic wave propagation at high altitudes (low pressures) is shown to be adiabatic, contrary to a suggestion by Golitsyn. An approximate treatment to include the effects of the finite depth of the atmosphere shows that the results are somewhat altered in detail. An important finding is that for this problem a non-gray atmosphere cannot be usefully approximated by one or more gray coefficients. A simple approximation to the effective absorption coefficient is suggested.
    publisherAmerican Meteorological Society
    titleAcoustic Wave Propagation in a Non-Gray Radiating Atmosphere
    typeJournal Paper
    journal volume25
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1968)025<0808:AWPIAN>2.0.CO;2
    journal fristpage808
    journal lastpage817
    treeJournal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 005
    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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