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    Systematic Design of Observational Arrays

    Source: Journal of Physical Oceanography:;1987:;Volume( 017 ):;issue: 007::page 885
    Author:
    McIntosh, Peter C.
    DOI: 10.1175/1520-0485(1987)017<0885:SDOOA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The variational data assimilation method of Bennett and McIntosh permits an assessment of the information content of observational arrays. This method relies on an approximate knowledge of the (linen) dynamics of the system, and on the instrument location, so that the efficiency arrays may be ascertained before deployment. The cumbersome trial-and-error optimization of array configuration may be circumvented by a careful study of the physics underlying the data assimilation procedure. As an example, array design criteria are developed for observing barotropic tides using tide gauges. In an open-ended channel, the variational method endeavors to synthesize the free modes of an infinite channel. Instruments should be located to facilitate the resolution of these modes. In a channel that is too small to support propagating Poincaré waves. tide gaups are best deployed along open sea boundaries where the amplitude of exponentially decaying Poincaré waves is largest. The maximum number of instruments contributing independent information depends both on the accuracy of the numerical modeling involved and on the data accuracy. Hence the desired numerical resolution may be used to determine the optimum number of measurements (for a given instrument uncertainty), or vice versa.
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      Systematic Design of Observational Arrays

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4164173
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    contributor authorMcIntosh, Peter C.
    date accessioned2017-06-09T14:48:25Z
    date available2017-06-09T14:48:25Z
    date copyright1987/07/01
    date issued1987
    identifier issn0022-3670
    identifier otherams-27195.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4164173
    description abstractThe variational data assimilation method of Bennett and McIntosh permits an assessment of the information content of observational arrays. This method relies on an approximate knowledge of the (linen) dynamics of the system, and on the instrument location, so that the efficiency arrays may be ascertained before deployment. The cumbersome trial-and-error optimization of array configuration may be circumvented by a careful study of the physics underlying the data assimilation procedure. As an example, array design criteria are developed for observing barotropic tides using tide gauges. In an open-ended channel, the variational method endeavors to synthesize the free modes of an infinite channel. Instruments should be located to facilitate the resolution of these modes. In a channel that is too small to support propagating Poincaré waves. tide gaups are best deployed along open sea boundaries where the amplitude of exponentially decaying Poincaré waves is largest. The maximum number of instruments contributing independent information depends both on the accuracy of the numerical modeling involved and on the data accuracy. Hence the desired numerical resolution may be used to determine the optimum number of measurements (for a given instrument uncertainty), or vice versa.
    publisherAmerican Meteorological Society
    titleSystematic Design of Observational Arrays
    typeJournal Paper
    journal volume17
    journal issue7
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/1520-0485(1987)017<0885:SDOOA>2.0.CO;2
    journal fristpage885
    journal lastpage902
    treeJournal of Physical Oceanography:;1987:;Volume( 017 ):;issue: 007
    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