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    Size Distributions and Dynamical Properties of Shallow Cumulus Clouds from Aircraft Observations and Satellite Data

    Source: Journal of the Atmospheric Sciences:;2003:;Volume( 060 ):;issue: 016::page 1895
    Author:
    Rodts, Stefaan M. A.
    ,
    Duynkerke, Peter G.
    ,
    Jonker, Harm J. J.
    DOI: 10.1175/1520-0469(2003)060<1895:SDADPO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: In this paper aircraft observations of shallow cumulus over Florida during the Small Cumulus Microphysics Study (SCMS) are analyzed. Size distributions of cloud fraction, mass flux, and in-cloud buoyancy flux are derived. These distributions provide information on the specific contribution of clouds with a certain horizontal size and reveal, for example, which size has the largest effect on cloud fraction or vertical transport. The analysis of four flights shows that the mass flux and buoyancy flux are dominated by intermediate-sized clouds (horizontal dimension of about 1 km). The cloud fraction, on the other hand, is found to be dominated by the smallest clouds observed. These clouds are additionally found to have a negative contribution to the mass flux, yet a positive contribution to the buoyancy flux. About 200 flight intersections of cumuli with horizontal sizes larger than 500 m are used to obtain average horizontal cross-section profiles of vertical velocity, liquid water content, liquid water potential temperature, and virtual potential temperature. A thin shell of descending air just around the cloud emerges as a conspicuous feature. Evidence is found that the descent is mainly caused by evaporative cooling, which results from lateral mixing at the cloud boundary. A Landsat satellite image near the flight region is analyzed to compare the cloud size distributions with the aircraft data. The cloud cover in the image appears to be dominated by much larger clouds than the aircraft observations indicated. To account for the different measurement methodology (two-dimensional versus one-dimensional) an equation with which one can predict the cloud size distribution that results from performing line measurements in a prescribed two-dimensional cumulus field is derived. The equation reveals that the aircraft cloud size distributions are always biased toward smaller cloud sizes. This effect is nevertheless not enough to reconcile the aircraft and satellite data, presumably because the analysis neglects the variability of clouds in the vertical direction.
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      Size Distributions and Dynamical Properties of Shallow Cumulus Clouds from Aircraft Observations and Satellite Data

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159847
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    contributor authorRodts, Stefaan M. A.
    contributor authorDuynkerke, Peter G.
    contributor authorJonker, Harm J. J.
    date accessioned2017-06-09T14:38:15Z
    date available2017-06-09T14:38:15Z
    date copyright2003/08/01
    date issued2003
    identifier issn0022-4928
    identifier otherams-23300.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159847
    description abstractIn this paper aircraft observations of shallow cumulus over Florida during the Small Cumulus Microphysics Study (SCMS) are analyzed. Size distributions of cloud fraction, mass flux, and in-cloud buoyancy flux are derived. These distributions provide information on the specific contribution of clouds with a certain horizontal size and reveal, for example, which size has the largest effect on cloud fraction or vertical transport. The analysis of four flights shows that the mass flux and buoyancy flux are dominated by intermediate-sized clouds (horizontal dimension of about 1 km). The cloud fraction, on the other hand, is found to be dominated by the smallest clouds observed. These clouds are additionally found to have a negative contribution to the mass flux, yet a positive contribution to the buoyancy flux. About 200 flight intersections of cumuli with horizontal sizes larger than 500 m are used to obtain average horizontal cross-section profiles of vertical velocity, liquid water content, liquid water potential temperature, and virtual potential temperature. A thin shell of descending air just around the cloud emerges as a conspicuous feature. Evidence is found that the descent is mainly caused by evaporative cooling, which results from lateral mixing at the cloud boundary. A Landsat satellite image near the flight region is analyzed to compare the cloud size distributions with the aircraft data. The cloud cover in the image appears to be dominated by much larger clouds than the aircraft observations indicated. To account for the different measurement methodology (two-dimensional versus one-dimensional) an equation with which one can predict the cloud size distribution that results from performing line measurements in a prescribed two-dimensional cumulus field is derived. The equation reveals that the aircraft cloud size distributions are always biased toward smaller cloud sizes. This effect is nevertheless not enough to reconcile the aircraft and satellite data, presumably because the analysis neglects the variability of clouds in the vertical direction.
    publisherAmerican Meteorological Society
    titleSize Distributions and Dynamical Properties of Shallow Cumulus Clouds from Aircraft Observations and Satellite Data
    typeJournal Paper
    journal volume60
    journal issue16
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2003)060<1895:SDADPO>2.0.CO;2
    journal fristpage1895
    journal lastpage1912
    treeJournal of the Atmospheric Sciences:;2003:;Volume( 060 ):;issue: 016
    contenttypeFulltext
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    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