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    Polarimetric Doppler Radar Observations of Kelvin–Helmholtz Waves in a Winter Storm

    Source: Journal of the Atmospheric Sciences:;2011:;Volume( 068 ):;issue: 008::page 1676
    Author:
    Houser, Jana Lesak
    ,
    Bluestein, Howard B.
    DOI: 10.1175/2011JAS3566.1
    Publisher: American Meteorological Society
    Abstract: elvin?Helmholtz waves were observed by the Twin Lakes, Oklahoma (KTLX), Weather Surveillance Radar-1988 Doppler (WSR-88D); the Norman, Oklahoma (KOUN), polarimetric WSR-88D; and the polarimetric Collaborative Adaptive Sensing of the Atmosphere (CASA) radars on 30 November 2006 during a winter storm in central Oklahoma. The life cycle and structure of the waves are analyzed from the radar data, and the nearby atmospheric conditions are examined. The initial perturbations associated with the waves are first evident only in the radars? radial velocity fields. As the waves mature, perturbations become discernable in the reflectivity factor Z and spectrum width (SW) fields of both radars, and in the differential reflectivity Zdr and, to a lesser extent, the cross-correlation coefficient ?hv fields of KOUN. As the waves break and begin to dissipate, the perturbations subside.A dual-Doppler analysis is synthesized to examine the kinematic structure of the waves and to relate the polarimetric observations to the kinematics. It is determined that Z and Zdr are enhanced in regions of upward motion (wave crests), and ?hv is reduced in the same vicinity and near the base of the wave circulations. Vertical velocity perturbations transport horizontal momentum upward and downward, inducing horizontal wind perturbations that are approximately 90° out of phase and downstream from their corresponding vertical velocity perturbations. Perturbations in Z, Zdr, and ?hv are observed in the vicinity of wave crests while SW perturbations occur predominately in and just upstream from wave troughs. It is determined that perturbations in the polarimetric variables are a result of the waves modifying local precipitation microphysics. Perturbations in Z and Zdr are hypothesized to be the result of columnar ice crystal generation whereas those in ?hv likely result from the mixing of ice crystals of various shapes and sizes. Perturbations in SW are a result of turbulent motions likely associated with wave breaking and downward advection of a strong shear layer.
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      Polarimetric Doppler Radar Observations of Kelvin–Helmholtz Waves in a Winter Storm

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4213599
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    contributor authorHouser, Jana Lesak
    contributor authorBluestein, Howard B.
    date accessioned2017-06-09T16:39:24Z
    date available2017-06-09T16:39:24Z
    date copyright2011/08/01
    date issued2011
    identifier issn0022-4928
    identifier otherams-71681.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4213599
    description abstractelvin?Helmholtz waves were observed by the Twin Lakes, Oklahoma (KTLX), Weather Surveillance Radar-1988 Doppler (WSR-88D); the Norman, Oklahoma (KOUN), polarimetric WSR-88D; and the polarimetric Collaborative Adaptive Sensing of the Atmosphere (CASA) radars on 30 November 2006 during a winter storm in central Oklahoma. The life cycle and structure of the waves are analyzed from the radar data, and the nearby atmospheric conditions are examined. The initial perturbations associated with the waves are first evident only in the radars? radial velocity fields. As the waves mature, perturbations become discernable in the reflectivity factor Z and spectrum width (SW) fields of both radars, and in the differential reflectivity Zdr and, to a lesser extent, the cross-correlation coefficient ?hv fields of KOUN. As the waves break and begin to dissipate, the perturbations subside.A dual-Doppler analysis is synthesized to examine the kinematic structure of the waves and to relate the polarimetric observations to the kinematics. It is determined that Z and Zdr are enhanced in regions of upward motion (wave crests), and ?hv is reduced in the same vicinity and near the base of the wave circulations. Vertical velocity perturbations transport horizontal momentum upward and downward, inducing horizontal wind perturbations that are approximately 90° out of phase and downstream from their corresponding vertical velocity perturbations. Perturbations in Z, Zdr, and ?hv are observed in the vicinity of wave crests while SW perturbations occur predominately in and just upstream from wave troughs. It is determined that perturbations in the polarimetric variables are a result of the waves modifying local precipitation microphysics. Perturbations in Z and Zdr are hypothesized to be the result of columnar ice crystal generation whereas those in ?hv likely result from the mixing of ice crystals of various shapes and sizes. Perturbations in SW are a result of turbulent motions likely associated with wave breaking and downward advection of a strong shear layer.
    publisherAmerican Meteorological Society
    titlePolarimetric Doppler Radar Observations of Kelvin–Helmholtz Waves in a Winter Storm
    typeJournal Paper
    journal volume68
    journal issue8
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/2011JAS3566.1
    journal fristpage1676
    journal lastpage1702
    treeJournal of the Atmospheric Sciences:;2011:;Volume( 068 ):;issue: 008
    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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