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    Global Brightness Temperature Spectra at High Wavenuinbers Utilizing Satellite Microwave Measurements

    Source: Journal of the Atmospheric Sciences:;1980:;Volume( 037 ):;issue: 005::page 1070
    Author:
    Stanford, John L.
    DOI: 10.1175/1520-0469(1980)037<1070:GBTSAH>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Satellite microwave brightness temperature (radiance) measurements represent weighted mean temperatures in a certain atmospheric layer. The high density of measurements along a polar-orbiting satellite track allows estimates of the brightness temperature variance spectrum at high meridional wavenumbers. Global data from the Nimbus 6 SCAMS microwave instrument sensitive to the 100?300 mb layer have been analyzed for 30 days in August 1975. The results reveal that the brightness temperature variance spectrum can be fit to the form km over the range k=22 to 59 (horizontal wavelengths 1800 to 700 km). Using 95% confidence intervals, the fit yields m = ?3.1±0.3 These results appear to have significance for estimates of energy cascade between different motion scales in the very high wavenumber regime.
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      Global Brightness Temperature Spectra at High Wavenuinbers Utilizing Satellite Microwave Measurements

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4153861
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    contributor authorStanford, John L.
    date accessioned2017-06-09T14:21:30Z
    date available2017-06-09T14:21:30Z
    date copyright1980/05/01
    date issued1980
    identifier issn0022-4928
    identifier otherams-17914.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153861
    description abstractSatellite microwave brightness temperature (radiance) measurements represent weighted mean temperatures in a certain atmospheric layer. The high density of measurements along a polar-orbiting satellite track allows estimates of the brightness temperature variance spectrum at high meridional wavenumbers. Global data from the Nimbus 6 SCAMS microwave instrument sensitive to the 100?300 mb layer have been analyzed for 30 days in August 1975. The results reveal that the brightness temperature variance spectrum can be fit to the form km over the range k=22 to 59 (horizontal wavelengths 1800 to 700 km). Using 95% confidence intervals, the fit yields m = ?3.1±0.3 These results appear to have significance for estimates of energy cascade between different motion scales in the very high wavenumber regime.
    publisherAmerican Meteorological Society
    titleGlobal Brightness Temperature Spectra at High Wavenuinbers Utilizing Satellite Microwave Measurements
    typeJournal Paper
    journal volume37
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1980)037<1070:GBTSAH>2.0.CO;2
    journal fristpage1070
    journal lastpage1076
    treeJournal of the Atmospheric Sciences:;1980:;Volume( 037 ):;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
    yabeshDSpacePersian