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    Plane Parallel Albedo Biases from Satellite Observations. Part II: Parameterizations for Bias Removal

    Source: Journal of Climate:;1998:;volume( 011 ):;issue: 005::page 933
    Author:
    Oreopoulos, Lazaros
    ,
    Davies, Roger
    DOI: 10.1175/1520-0442(1998)011<0933:PPABFS>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Using the same satellite observations as in Part I of this paper, the authors explore ways to remove the cloud albedo bias (or plane parallel albedo bias), the difference between the plane parallel homogeneous albedo and the average albedo of independent pixels, in regions similar in size to climate model grid boxes. Scaling regional mean optical depths with the reduction factor of R. F. Cahalan et al. provides albedos close to the independent pixel values. Computed albedos approach the independent pixel values within 0.01 for ?40% of the regions tested and give standard deviations ?0.02?0.04. Fitting lognormal distributions to the observed optical depth distributions gives albedos within 0.01 of the independent pixel values more than 70% of the time, with standard deviations ?0.02?0.06. Gamma distributions are less successful than lognormal distributions, giving acceptable results (average bias ?0.01?0.02, standard deviation ?0.05?0.08) only when their parameters are estimated from the maximum likelihood estimates method. The poor performance of the gamma distribution when the method of moments is used for parameter estimation (as H. W. Barker et al. did) is attributed to the presence of high optical depth values in our retrieved fields. To apply any of the above corrections in GCMs, quantities that are not presently provided by these models are required. The reduction factor and ?gamma IP? method require the mean logarithm of optical depth, whereas the lognormal method also requires the variance. The authors suggest a parameterization of these quantities in terms of mean optical depth and cloud fraction, variables available in most GCMs. The albedos resulting from the parameterized versions of the correction methods are still much closer to the independent pixel values than the albedos of the plane parallel homogeneous assumption. Although the ?lognormal IP? gives the best overall performance, it requires knowledge of two logarithmic moments and numerical integration. It may therefore prove more appealing for observational than modeling applications.
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      Plane Parallel Albedo Biases from Satellite Observations. Part II: Parameterizations for Bias Removal

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4189133
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    contributor authorOreopoulos, Lazaros
    contributor authorDavies, Roger
    date accessioned2017-06-09T15:38:57Z
    date available2017-06-09T15:38:57Z
    date copyright1998/05/01
    date issued1998
    identifier issn0894-8755
    identifier otherams-4966.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4189133
    description abstractUsing the same satellite observations as in Part I of this paper, the authors explore ways to remove the cloud albedo bias (or plane parallel albedo bias), the difference between the plane parallel homogeneous albedo and the average albedo of independent pixels, in regions similar in size to climate model grid boxes. Scaling regional mean optical depths with the reduction factor of R. F. Cahalan et al. provides albedos close to the independent pixel values. Computed albedos approach the independent pixel values within 0.01 for ?40% of the regions tested and give standard deviations ?0.02?0.04. Fitting lognormal distributions to the observed optical depth distributions gives albedos within 0.01 of the independent pixel values more than 70% of the time, with standard deviations ?0.02?0.06. Gamma distributions are less successful than lognormal distributions, giving acceptable results (average bias ?0.01?0.02, standard deviation ?0.05?0.08) only when their parameters are estimated from the maximum likelihood estimates method. The poor performance of the gamma distribution when the method of moments is used for parameter estimation (as H. W. Barker et al. did) is attributed to the presence of high optical depth values in our retrieved fields. To apply any of the above corrections in GCMs, quantities that are not presently provided by these models are required. The reduction factor and ?gamma IP? method require the mean logarithm of optical depth, whereas the lognormal method also requires the variance. The authors suggest a parameterization of these quantities in terms of mean optical depth and cloud fraction, variables available in most GCMs. The albedos resulting from the parameterized versions of the correction methods are still much closer to the independent pixel values than the albedos of the plane parallel homogeneous assumption. Although the ?lognormal IP? gives the best overall performance, it requires knowledge of two logarithmic moments and numerical integration. It may therefore prove more appealing for observational than modeling applications.
    publisherAmerican Meteorological Society
    titlePlane Parallel Albedo Biases from Satellite Observations. Part II: Parameterizations for Bias Removal
    typeJournal Paper
    journal volume11
    journal issue5
    journal titleJournal of Climate
    identifier doi10.1175/1520-0442(1998)011<0933:PPABFS>2.0.CO;2
    journal fristpage933
    journal lastpage944
    treeJournal of Climate:;1998:;volume( 011 ):;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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