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    Effects of Cloud Horizontal Inhomogeneity on the Optical Thickness Retrieved from Moderate-Resolution Satellite Data

    Source: Journal of the Atmospheric Sciences:;2002:;Volume( 059 ):;issue: 014::page 2227
    Author:
    Iwabuchi, Hironobu
    ,
    Hayasaka, Tadahiro
    DOI: 10.1175/1520-0469(2002)059<2227:EOCHIO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Cloud remote sensing techniques are conventionally based on the independent pixel approximation (IPA). Here, three-dimensional (3D) radiative effects on IPA-based retrieved optical thickness from a visible-wavelength moderate-resolution (about 1 km) sensor are investigated. A Monte Carlo 3D radiative transfer model and a lognormal spectral cloud model are used to simulate monochromatic radiance reflected from overcast boundary layer cloud. A characterization of statistical properties of the optical thickness by the mean (M) and variance (S2) of the logarithm of the optical thickness is proposed, where S represents a degree of cloud inhomogeneity. Biases in retrieved values of the two parameters with the IPA are defined as ?M and ?S2 and attributed to neglect of net horizontal radiative transport in the IPA. Sensitivities of ?M and ?S2 are tested with respect to geometrical roughness, M, S, mean geometrical thickness, spectral exponent of optical thickness fluctuation, ground surface reflectance, and bidirectional angles. The 3D radiative effects are sensitive to the geometrical roughness of cloud top rather than internal inhomogeneity of the extinction coefficient. The bias ?M is negative in forward scattering viewing geometry due to cloud-side shadowing, while positive in backscattering viewing geometry due to side illumination. It is found that ?M is proportional to S2 and large for a dense cloud. On the other hand, ?S2 largely depends on the solar zenith angle; smoothing is exhibited for high solar elevation and roughening for low solar elevation. The smoothing and roughening phenomena are found to be almost independent of the inhomogeneity parameter. An optically thick cloud exhibits more roughening, while for a geometrically thick cloud both smoothing and roughening are enhanced. It is suggested that for the bias removal some empirical assumptions are required in geometrical and microphysical properties of cloud, which should be studied with in situ observation data.
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      Effects of Cloud Horizontal Inhomogeneity on the Optical Thickness Retrieved from Moderate-Resolution Satellite Data

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159675
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    contributor authorIwabuchi, Hironobu
    contributor authorHayasaka, Tadahiro
    date accessioned2017-06-09T14:37:47Z
    date available2017-06-09T14:37:47Z
    date copyright2002/07/01
    date issued2002
    identifier issn0022-4928
    identifier otherams-23146.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159675
    description abstractCloud remote sensing techniques are conventionally based on the independent pixel approximation (IPA). Here, three-dimensional (3D) radiative effects on IPA-based retrieved optical thickness from a visible-wavelength moderate-resolution (about 1 km) sensor are investigated. A Monte Carlo 3D radiative transfer model and a lognormal spectral cloud model are used to simulate monochromatic radiance reflected from overcast boundary layer cloud. A characterization of statistical properties of the optical thickness by the mean (M) and variance (S2) of the logarithm of the optical thickness is proposed, where S represents a degree of cloud inhomogeneity. Biases in retrieved values of the two parameters with the IPA are defined as ?M and ?S2 and attributed to neglect of net horizontal radiative transport in the IPA. Sensitivities of ?M and ?S2 are tested with respect to geometrical roughness, M, S, mean geometrical thickness, spectral exponent of optical thickness fluctuation, ground surface reflectance, and bidirectional angles. The 3D radiative effects are sensitive to the geometrical roughness of cloud top rather than internal inhomogeneity of the extinction coefficient. The bias ?M is negative in forward scattering viewing geometry due to cloud-side shadowing, while positive in backscattering viewing geometry due to side illumination. It is found that ?M is proportional to S2 and large for a dense cloud. On the other hand, ?S2 largely depends on the solar zenith angle; smoothing is exhibited for high solar elevation and roughening for low solar elevation. The smoothing and roughening phenomena are found to be almost independent of the inhomogeneity parameter. An optically thick cloud exhibits more roughening, while for a geometrically thick cloud both smoothing and roughening are enhanced. It is suggested that for the bias removal some empirical assumptions are required in geometrical and microphysical properties of cloud, which should be studied with in situ observation data.
    publisherAmerican Meteorological Society
    titleEffects of Cloud Horizontal Inhomogeneity on the Optical Thickness Retrieved from Moderate-Resolution Satellite Data
    typeJournal Paper
    journal volume59
    journal issue14
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2002)059<2227:EOCHIO>2.0.CO;2
    journal fristpage2227
    journal lastpage2242
    treeJournal of the Atmospheric Sciences:;2002:;Volume( 059 ):;issue: 014
    contenttypeFulltext
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian
     
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian