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    The “Mad Sea” Phenomenon in the Strait of Sicily

    Source: Journal of Physical Oceanography:;1999:;Volume( 029 ):;issue: 009::page 2210
    Author:
    Candela, Julio
    ,
    Mazzola, Salvatore
    ,
    Sammari, Chérif
    ,
    Limeburner, Richard
    ,
    Lozano, Carlos J.
    ,
    Patti, Bernardo
    ,
    Bonanno, Angelo
    DOI: 10.1175/1520-0485(1999)029<2210:TMSPIT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Sea level observations at Cape Bon, Tunisia, and Mazara del Vallo, Sicily, show that large, coherent oscillations exist across the Strait of Sicily with significant energy bands centered at periods of 35.3, 41.6, 50.6, 75.8, and 134.5 min, whose possible structure is confirmed by a numerical approximation to the gravitational barotropic normal modes with realistic topography. It is observed that these oscillations are related to the passage of synoptic weather systems over the region. An investigation on the configuration, phase velocity, and direction of approach of atmospheric disturbances over the region suggests that the oscillations in the Strait of Sicily could be forced by instabilities that develop in large-scale, low pressure fronts that propagate as pressure gravity waves with an approximate phase speed between 24 and 30 m s?1.
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      The “Mad Sea” Phenomenon in the Strait of Sicily

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4166299
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    contributor authorCandela, Julio
    contributor authorMazzola, Salvatore
    contributor authorSammari, Chérif
    contributor authorLimeburner, Richard
    contributor authorLozano, Carlos J.
    contributor authorPatti, Bernardo
    contributor authorBonanno, Angelo
    date accessioned2017-06-09T14:53:39Z
    date available2017-06-09T14:53:39Z
    date copyright1999/09/01
    date issued1999
    identifier issn0022-3670
    identifier otherams-29108.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4166299
    description abstractSea level observations at Cape Bon, Tunisia, and Mazara del Vallo, Sicily, show that large, coherent oscillations exist across the Strait of Sicily with significant energy bands centered at periods of 35.3, 41.6, 50.6, 75.8, and 134.5 min, whose possible structure is confirmed by a numerical approximation to the gravitational barotropic normal modes with realistic topography. It is observed that these oscillations are related to the passage of synoptic weather systems over the region. An investigation on the configuration, phase velocity, and direction of approach of atmospheric disturbances over the region suggests that the oscillations in the Strait of Sicily could be forced by instabilities that develop in large-scale, low pressure fronts that propagate as pressure gravity waves with an approximate phase speed between 24 and 30 m s?1.
    publisherAmerican Meteorological Society
    titleThe “Mad Sea” Phenomenon in the Strait of Sicily
    typeJournal Paper
    journal volume29
    journal issue9
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/1520-0485(1999)029<2210:TMSPIT>2.0.CO;2
    journal fristpage2210
    journal lastpage2231
    treeJournal of Physical Oceanography:;1999:;Volume( 029 ):;issue: 009
    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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