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    Determination of the Shortwave Anisotropic Function for Clear-Sky Desert Scenes from Meteosat Data

    Source: Journal of Applied Meteorology:;1995:;volume( 034 ):;issue: 006::page 1349
    Author:
    Capderou, Michel
    ,
    Kandel, Robert
    DOI: 10.1175/1520-0450(1995)034<1349:DOTSAF>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Determination of planetary albedo on the basis of satellite observations of reflected shortwave (SW) radiances requires taking into account the anisotropic (non-Lambertian) reflectance properties of the earth?atmosphere system, depending both on the cloud cover and the nature of the underlying, surface. One approach frequently used has been to represent these properties by a limited set of normalized bidirectional reflectance functions (BDRF) for different scene types. The construction of the normalized BDRFs used to process the Earth Radiation Budget Experiment (ERBE) measurements was based mostly on data from the sun-synchronous Nimbus-7 mission, observing close to local noon. Consequently, because desert zones are fairly restricted in latitude, only a small range of solar zenith angles was sampled. Here the authors consider, for clear-sky desert areas, the improvements that can be made using data from the geostationary satellite Meteosat, which samples all solar zenith angles that occur. The authors define BDRF ratios (between two instants on the same day for the same area) that depend on viewing geometry (five angles for a geostationary satellite) and that together with infrared window radiance measurements allow to distinguish clear and cloudy desert scenes. Using three to five Meteosat images per day over the year 1985, and considering 42 areas in desert zones, the authors compute roughly 12 500 clear-sky BDRF ratios (representing 4.5 million B2 pixels), and sort these into bins in five-dimensional angular space. Values of the BDRF ratio are well defined and stable in each of these bins. Application of the Helmholtz reciprocity principle yields data for angular bins not directly observed. After spectral corrections and normalizations, the authors obtain a completely defined SW angular model (i.e., normalized anisotropic function and directional albedo) for clear-sky desert scenes. This model is quite different from that used in the ERBE analyses. The authors discuss the improvements obtained.
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      Determination of the Shortwave Anisotropic Function for Clear-Sky Desert Scenes from Meteosat Data

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4147463
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    contributor authorCapderou, Michel
    contributor authorKandel, Robert
    date accessioned2017-06-09T14:05:13Z
    date available2017-06-09T14:05:13Z
    date copyright1995/06/01
    date issued1995
    identifier issn0894-8763
    identifier otherams-12155.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4147463
    description abstractDetermination of planetary albedo on the basis of satellite observations of reflected shortwave (SW) radiances requires taking into account the anisotropic (non-Lambertian) reflectance properties of the earth?atmosphere system, depending both on the cloud cover and the nature of the underlying, surface. One approach frequently used has been to represent these properties by a limited set of normalized bidirectional reflectance functions (BDRF) for different scene types. The construction of the normalized BDRFs used to process the Earth Radiation Budget Experiment (ERBE) measurements was based mostly on data from the sun-synchronous Nimbus-7 mission, observing close to local noon. Consequently, because desert zones are fairly restricted in latitude, only a small range of solar zenith angles was sampled. Here the authors consider, for clear-sky desert areas, the improvements that can be made using data from the geostationary satellite Meteosat, which samples all solar zenith angles that occur. The authors define BDRF ratios (between two instants on the same day for the same area) that depend on viewing geometry (five angles for a geostationary satellite) and that together with infrared window radiance measurements allow to distinguish clear and cloudy desert scenes. Using three to five Meteosat images per day over the year 1985, and considering 42 areas in desert zones, the authors compute roughly 12 500 clear-sky BDRF ratios (representing 4.5 million B2 pixels), and sort these into bins in five-dimensional angular space. Values of the BDRF ratio are well defined and stable in each of these bins. Application of the Helmholtz reciprocity principle yields data for angular bins not directly observed. After spectral corrections and normalizations, the authors obtain a completely defined SW angular model (i.e., normalized anisotropic function and directional albedo) for clear-sky desert scenes. This model is quite different from that used in the ERBE analyses. The authors discuss the improvements obtained.
    publisherAmerican Meteorological Society
    titleDetermination of the Shortwave Anisotropic Function for Clear-Sky Desert Scenes from Meteosat Data
    typeJournal Paper
    journal volume34
    journal issue6
    journal titleJournal of Applied Meteorology
    identifier doi10.1175/1520-0450(1995)034<1349:DOTSAF>2.0.CO;2
    journal fristpage1349
    journal lastpage1374
    treeJournal of Applied Meteorology:;1995:;volume( 034 ):;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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