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    A Comparison of Cyclonic Ring Structures in the Northern Sargasso Sea

    Source: Journal of Physical Oceanography:;1978:;Volume( 008 ):;issue: 006::page 997
    Author:
    Hagan, Denise E.
    ,
    Olson, Donald B.
    ,
    Schmitz, Joyce E.
    ,
    Vastano, Andrew C.
    DOI: 10.1175/1520-0485(1978)008<0997:ACOCRS>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Field observations provide a data base that supports a comparison of ring structures in terms of the background Sargasso Sea environment. Five ring surveys, three from the 1967 sequence, a big baby ring and ring AL, were selected for this study. Anomalies of temperature, salinity, transport potential energy density, heat content and sound velocity have been examined using a reference which closely approximates Iselin's characteristic T-S relation for the western gyre. The results for the 1967 sequence demonstrate an initial reduction in anomaly strengths followed by strong ring stability. Comparison of two different rings, possibly equal in age, show the effect of the initial water mass conditions on anomaly strengths. Comparison of a cyclonic ring and the big baby ring reveals similar anomaly strengths and sizes in the same geographical region for rings that are assumed to be two and eleven months in age, respectively. This suggests that big baby rings can initially represent more intense perturbations to the Sargasso Sea than cyclonic ring counterparts.
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      A Comparison of Cyclonic Ring Structures in the Northern Sargasso Sea

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4162694
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    • Journal of Physical Oceanography

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    contributor authorHagan, Denise E.
    contributor authorOlson, Donald B.
    contributor authorSchmitz, Joyce E.
    contributor authorVastano, Andrew C.
    date accessioned2017-06-09T14:44:53Z
    date available2017-06-09T14:44:53Z
    date copyright1978/11/01
    date issued1978
    identifier issn0022-3670
    identifier otherams-25864.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4162694
    description abstractField observations provide a data base that supports a comparison of ring structures in terms of the background Sargasso Sea environment. Five ring surveys, three from the 1967 sequence, a big baby ring and ring AL, were selected for this study. Anomalies of temperature, salinity, transport potential energy density, heat content and sound velocity have been examined using a reference which closely approximates Iselin's characteristic T-S relation for the western gyre. The results for the 1967 sequence demonstrate an initial reduction in anomaly strengths followed by strong ring stability. Comparison of two different rings, possibly equal in age, show the effect of the initial water mass conditions on anomaly strengths. Comparison of a cyclonic ring and the big baby ring reveals similar anomaly strengths and sizes in the same geographical region for rings that are assumed to be two and eleven months in age, respectively. This suggests that big baby rings can initially represent more intense perturbations to the Sargasso Sea than cyclonic ring counterparts.
    publisherAmerican Meteorological Society
    titleA Comparison of Cyclonic Ring Structures in the Northern Sargasso Sea
    typeJournal Paper
    journal volume8
    journal issue6
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/1520-0485(1978)008<0997:ACOCRS>2.0.CO;2
    journal fristpage997
    journal lastpage1008
    treeJournal of Physical Oceanography:;1978:;Volume( 008 ):;issue: 006
    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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