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    Lunar Tidal Winds Measured in the Upper Atmosphere (78–105 km) at Saskatoon, Canada

    Source: Journal of the Atmospheric Sciences:;1987:;Volume( 044 ):;issue: 008::page 1143
    Author:
    Stening, R. J.
    ,
    Meek, C. E.
    ,
    Manson, A. H.
    DOI: 10.1175/1520-0469(1987)044<1143:LTWMIT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Six years of winds data measured by the partial reflection drifts technique have been analyzed for lunar tides. Data are available at 3 km intervals of height and are separately analyzed in two year datasets to cheek consistency. A month-by-month seasonal variation is derived. Largest amplitudes of the lunar tide occur in January?February with a smaller maximum in summer. The vertical wavelength is longest in summer, and the tide then resembles that predicted for a pure (2, 2) mode. In winter vertical wavelengths range from 25 to 81 km in different years. Several of these results do not agree with the model of Forbes. An O1 component of the lunar tide could not be detected.
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      Lunar Tidal Winds Measured in the Upper Atmosphere (78–105 km) at Saskatoon, Canada

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4155648
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    contributor authorStening, R. J.
    contributor authorMeek, C. E.
    contributor authorManson, A. H.
    date accessioned2017-06-09T14:27:15Z
    date available2017-06-09T14:27:15Z
    date copyright1987/04/01
    date issued1987
    identifier issn0022-4928
    identifier otherams-19522.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4155648
    description abstractSix years of winds data measured by the partial reflection drifts technique have been analyzed for lunar tides. Data are available at 3 km intervals of height and are separately analyzed in two year datasets to cheek consistency. A month-by-month seasonal variation is derived. Largest amplitudes of the lunar tide occur in January?February with a smaller maximum in summer. The vertical wavelength is longest in summer, and the tide then resembles that predicted for a pure (2, 2) mode. In winter vertical wavelengths range from 25 to 81 km in different years. Several of these results do not agree with the model of Forbes. An O1 component of the lunar tide could not be detected.
    publisherAmerican Meteorological Society
    titleLunar Tidal Winds Measured in the Upper Atmosphere (78–105 km) at Saskatoon, Canada
    typeJournal Paper
    journal volume44
    journal issue8
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1987)044<1143:LTWMIT>2.0.CO;2
    journal fristpage1143
    journal lastpage1151
    treeJournal of the Atmospheric Sciences:;1987:;Volume( 044 ):;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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