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    Diurnal Tidal Motions between 30 and 60 Kilometers in Summer

    Source: Journal of the Atmospheric Sciences:;1966:;Volume( 023 ):;issue: 004::page 416
    Author:
    Reed, Richard J.
    ,
    McKenzie, Donald J.
    ,
    Vyverberg, Joan V.
    DOI: 10.1175/1520-0469(1966)023<0416:DTMBAK>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Routine wind observations for nine Meteorological Rocket Network stations located between 88 and 64N are examined for evidence of diurnal tidal motions. Only the behavior of the meridional component in summer is considered. The amplitude of this component is found to be small (about 1 m sec?1) below 40 km, to increase rapidly near 45 km, and to achieve a maximum value of 5?8 m sec?1 or somewhat above, 50 km. Between 55 and 60 km the amplitude diminishes slightly, while higher up it appears, from the meager data available, that a further increase takes place. At the Northern Hemisphere stations the maximum south wind occurs at about noon near 50 km and two or three hours later several kilometers below. There is evidence of a pronounced semidiurnal oscillation above 55 km at Ascension Island (8S). A global model of the diurnal tidal motions, based in part on observation and in part on theory, is presented. The proposed instantaneous motions are tangential to great circle arcs which connect the point on the equator, where it is local noon, to its conjugate point, The vertical motion is upward in the vicinity of the former point, giving adiabatic cooling around noon. Subsidence and adiabatic warming occur about the conjugate point on the dark side of the earth.
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      Diurnal Tidal Motions between 30 and 60 Kilometers in Summer

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4150864
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    contributor authorReed, Richard J.
    contributor authorMcKenzie, Donald J.
    contributor authorVyverberg, Joan V.
    date accessioned2017-06-09T14:13:51Z
    date available2017-06-09T14:13:51Z
    date copyright1966/07/01
    date issued1966
    identifier issn0022-4928
    identifier otherams-15216.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150864
    description abstractRoutine wind observations for nine Meteorological Rocket Network stations located between 88 and 64N are examined for evidence of diurnal tidal motions. Only the behavior of the meridional component in summer is considered. The amplitude of this component is found to be small (about 1 m sec?1) below 40 km, to increase rapidly near 45 km, and to achieve a maximum value of 5?8 m sec?1 or somewhat above, 50 km. Between 55 and 60 km the amplitude diminishes slightly, while higher up it appears, from the meager data available, that a further increase takes place. At the Northern Hemisphere stations the maximum south wind occurs at about noon near 50 km and two or three hours later several kilometers below. There is evidence of a pronounced semidiurnal oscillation above 55 km at Ascension Island (8S). A global model of the diurnal tidal motions, based in part on observation and in part on theory, is presented. The proposed instantaneous motions are tangential to great circle arcs which connect the point on the equator, where it is local noon, to its conjugate point, The vertical motion is upward in the vicinity of the former point, giving adiabatic cooling around noon. Subsidence and adiabatic warming occur about the conjugate point on the dark side of the earth.
    publisherAmerican Meteorological Society
    titleDiurnal Tidal Motions between 30 and 60 Kilometers in Summer
    typeJournal Paper
    journal volume23
    journal issue4
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1966)023<0416:DTMBAK>2.0.CO;2
    journal fristpage416
    journal lastpage423
    treeJournal of the Atmospheric Sciences:;1966:;Volume( 023 ):;issue: 004
    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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