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    The Structure of Winds of the Upper Troposphere at Mesoscale

    Source: Journal of the Atmospheric Sciences:;1963:;Volume( 020 ):;issue: 002::page 94
    Author:
    Mantis, Homer T.
    DOI: 10.1175/1520-0469(1963)020<0094:TSOWOT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Spectra of the variance of horizontal velocities derived from the trajectories of superpressure altitude-controlled balloons have been obtained in the frequency range 0.005 to 0.5 cy min?1. With the aid of other constant-altitude balloon data, a spectrum of velocity variance of the upper tropospheric winds is proposed for a range of frequencies termed mesoscale, which is meant to describe scales of motion just smaller than synoptic scale but larger than the motions usually referred to as turbulence. The mesoscale spectra all decreases sharply with frequency at frequencies just above synoptic scale to a frequency of about 0.1 cy min?1, where an irregular increase sets in. The spectra continue to rise to the highest frequencies analyzed, pointing to a second spectral maximum in the turbulent regime. The spectra have been used to estimate the non-representative mesoscale standard deviation of the upper winds of 7 to 17 knots. A horizontal diffusivity by mesoscale motions is estimated to be of the order of 102 cm2 see?1.
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      The Structure of Winds of the Upper Troposphere at Mesoscale

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4150499
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    contributor authorMantis, Homer T.
    date accessioned2017-06-09T14:12:59Z
    date available2017-06-09T14:12:59Z
    date copyright1963/03/01
    date issued1963
    identifier issn0022-4928
    identifier otherams-14889.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150499
    description abstractSpectra of the variance of horizontal velocities derived from the trajectories of superpressure altitude-controlled balloons have been obtained in the frequency range 0.005 to 0.5 cy min?1. With the aid of other constant-altitude balloon data, a spectrum of velocity variance of the upper tropospheric winds is proposed for a range of frequencies termed mesoscale, which is meant to describe scales of motion just smaller than synoptic scale but larger than the motions usually referred to as turbulence. The mesoscale spectra all decreases sharply with frequency at frequencies just above synoptic scale to a frequency of about 0.1 cy min?1, where an irregular increase sets in. The spectra continue to rise to the highest frequencies analyzed, pointing to a second spectral maximum in the turbulent regime. The spectra have been used to estimate the non-representative mesoscale standard deviation of the upper winds of 7 to 17 knots. A horizontal diffusivity by mesoscale motions is estimated to be of the order of 102 cm2 see?1.
    publisherAmerican Meteorological Society
    titleThe Structure of Winds of the Upper Troposphere at Mesoscale
    typeJournal Paper
    journal volume20
    journal issue2
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1963)020<0094:TSOWOT>2.0.CO;2
    journal fristpage94
    journal lastpage106
    treeJournal of the Atmospheric Sciences:;1963:;Volume( 020 ):;issue: 002
    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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