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    Effects of Spectral Truncation on General Circulation and Long-Range Prediction

    Source: Journal of the Atmospheric Sciences:;1971:;Volume( 028 ):;issue: 004::page 457
    Author:
    Baer, F.
    ,
    Alyea, F. N.
    DOI: 10.1175/1520-0469(1971)028<0457:EOSTOG>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Although atmospheric prediction models appear to yield results similar to observation, both their detailed predictive capability and their time-averaged forecasts depend on space truncation. Such dependence may be readily studied with a spectral model because of the ease of modifying truncation. A simple, two-level, quasi-geostrophic, forced general circulation model was represented in spectral form and nine cases of different truncation were integrated for the same forcing, starting with initial conditions generated from a state of rest. The truncations ranged from six to sixteen meridional waves, from five to ten degrees of freedom with latitude, and the models were integrated for about 60 days with finite-amplitude nonlinearity. Considering the kinetic energy in the vertical mean flow, and separating this energy into zonal and eddy, the results show that the general circulation may be predicted with as few as twelve planetary waves and eight latitudinal degrees of freedom, whereas detailed prediction for a period of 15?20 days requires at least sixteen planetary waves and eight to ten latitudinal degrees of freedom. The broad variation in solutions for different truncations observed in this study implies that care must be taken in selecting space truncation for any physical model chosen for integration.
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      Effects of Spectral Truncation on General Circulation and Long-Range Prediction

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4151683
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    contributor authorBaer, F.
    contributor authorAlyea, F. N.
    date accessioned2017-06-09T14:15:49Z
    date available2017-06-09T14:15:49Z
    date copyright1971/05/01
    date issued1971
    identifier issn0022-4928
    identifier otherams-15954.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151683
    description abstractAlthough atmospheric prediction models appear to yield results similar to observation, both their detailed predictive capability and their time-averaged forecasts depend on space truncation. Such dependence may be readily studied with a spectral model because of the ease of modifying truncation. A simple, two-level, quasi-geostrophic, forced general circulation model was represented in spectral form and nine cases of different truncation were integrated for the same forcing, starting with initial conditions generated from a state of rest. The truncations ranged from six to sixteen meridional waves, from five to ten degrees of freedom with latitude, and the models were integrated for about 60 days with finite-amplitude nonlinearity. Considering the kinetic energy in the vertical mean flow, and separating this energy into zonal and eddy, the results show that the general circulation may be predicted with as few as twelve planetary waves and eight latitudinal degrees of freedom, whereas detailed prediction for a period of 15?20 days requires at least sixteen planetary waves and eight to ten latitudinal degrees of freedom. The broad variation in solutions for different truncations observed in this study implies that care must be taken in selecting space truncation for any physical model chosen for integration.
    publisherAmerican Meteorological Society
    titleEffects of Spectral Truncation on General Circulation and Long-Range Prediction
    typeJournal Paper
    journal volume28
    journal issue4
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1971)028<0457:EOSTOG>2.0.CO;2
    journal fristpage457
    journal lastpage481
    treeJournal of the Atmospheric Sciences:;1971:;Volume( 028 ):;issue: 004
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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