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    Inertia–Gravity Waves Observed in the Lower Stratosphere over Macquarie Island

    Source: Journal of the Atmospheric Sciences:;2000:;Volume( 057 ):;issue: 005::page 737
    Author:
    Guest, Fiona M.
    ,
    Reeder, Michael J.
    ,
    Marks, Crispin J.
    ,
    Karoly, David J.
    DOI: 10.1175/1520-0469(2000)057<0737:IGWOIT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: This study examines the properties of inertia?gravity waves observed in the lower stratosphere over Macquarie Island, how these properties vary with season, and the likely source of the waves. The waves are observed in high-resolution upper-air ozonesonde soundings of wind and temperature released from Macquarie Island during the 1994 ASHOE?MAESA program. The properties of the inertia?gravity waves observed in the soundings are quantified using hodograph and rotary spectral analyses. The analyzed waves have horizontal wavelengths between 100 and 1000 km, vertical wavelengths between about 1 and 7 km, intrinsic frequencies between f and 2f, and horizontal trace speeds between ?50 and 30 m s?1. There appears to be a seasonal cycle in the inertia?gravity wave activity in the lower stratosphere, the minimum being in the austral winter when the background zonal flow is strong and westerly and its vertical shear is positive. In contrast, the variance of the horizontal perturbation winds does not show a similar seasonal cycle. Inertia?gravity waves are detected over Macquarie Island on days with a common synoptic pattern. Two features define this synoptic pattern: 1) an upper-level jet and associated surface front lying upstream of Macquarie Island, and 2) a 300-hPa height field with Macquarie Island located between the inflection axis and the downstream ridge. This common synoptic pattern is observed on 16 of the 21 days on which inertia?gravity waves were detected. Moreover, the pattern is not observed on 15 of the 21 days in which inertia?gravity waves are not identified. This common synoptic pattern shows a seasonal cycle similar to that found for the inertia?gravity wave activity. Analyses of the ozonesonde soundings suggest also that the source of the inertia?gravity waves is in the troposphere. Using GROGRAT, the ray-tracing model developed by Marks and Eckermann, a cone of rays is released 21 km above Macquarie Island and traced backward in time. These rays suggest that the inertia?gravity waves are generated in the jet?front system southwest of Macquarie Island.
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      Inertia–Gravity Waves Observed in the Lower Stratosphere over Macquarie Island

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159017
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    • Journal of the Atmospheric Sciences

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    contributor authorGuest, Fiona M.
    contributor authorReeder, Michael J.
    contributor authorMarks, Crispin J.
    contributor authorKaroly, David J.
    date accessioned2017-06-09T14:36:01Z
    date available2017-06-09T14:36:01Z
    date copyright2000/03/01
    date issued2000
    identifier issn0022-4928
    identifier otherams-22554.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159017
    description abstractThis study examines the properties of inertia?gravity waves observed in the lower stratosphere over Macquarie Island, how these properties vary with season, and the likely source of the waves. The waves are observed in high-resolution upper-air ozonesonde soundings of wind and temperature released from Macquarie Island during the 1994 ASHOE?MAESA program. The properties of the inertia?gravity waves observed in the soundings are quantified using hodograph and rotary spectral analyses. The analyzed waves have horizontal wavelengths between 100 and 1000 km, vertical wavelengths between about 1 and 7 km, intrinsic frequencies between f and 2f, and horizontal trace speeds between ?50 and 30 m s?1. There appears to be a seasonal cycle in the inertia?gravity wave activity in the lower stratosphere, the minimum being in the austral winter when the background zonal flow is strong and westerly and its vertical shear is positive. In contrast, the variance of the horizontal perturbation winds does not show a similar seasonal cycle. Inertia?gravity waves are detected over Macquarie Island on days with a common synoptic pattern. Two features define this synoptic pattern: 1) an upper-level jet and associated surface front lying upstream of Macquarie Island, and 2) a 300-hPa height field with Macquarie Island located between the inflection axis and the downstream ridge. This common synoptic pattern is observed on 16 of the 21 days on which inertia?gravity waves were detected. Moreover, the pattern is not observed on 15 of the 21 days in which inertia?gravity waves are not identified. This common synoptic pattern shows a seasonal cycle similar to that found for the inertia?gravity wave activity. Analyses of the ozonesonde soundings suggest also that the source of the inertia?gravity waves is in the troposphere. Using GROGRAT, the ray-tracing model developed by Marks and Eckermann, a cone of rays is released 21 km above Macquarie Island and traced backward in time. These rays suggest that the inertia?gravity waves are generated in the jet?front system southwest of Macquarie Island.
    publisherAmerican Meteorological Society
    titleInertia–Gravity Waves Observed in the Lower Stratosphere over Macquarie Island
    typeJournal Paper
    journal volume57
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2000)057<0737:IGWOIT>2.0.CO;2
    journal fristpage737
    journal lastpage752
    treeJournal of the Atmospheric Sciences:;2000:;Volume( 057 ):;issue: 005
    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
    yabeshDSpacePersian