YaBeSH Engineering and Technology Library

    • Journals
    • PaperQuest
    • YSE Standards
    • YaBeSH
    • Login
    View Item 
    •   YE&T Library
    • AMS
    • Journal of the Atmospheric Sciences
    • View Item
    •   YE&T Library
    • AMS
    • Journal of the Atmospheric Sciences
    • View Item
    • All Fields
    • Source Title
    • Year
    • Publisher
    • Title
    • Subject
    • Author
    • DOI
    • ISBN
    Advanced Search
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Archive

    A Numerical Study of the Interaction between Stationary Rossby Waves and Eastward-Traveling Waves in the Southern Hemisphere Stratosphere

    Source: Journal of the Atmospheric Sciences:;1992:;Volume( 049 ):;issue: 015::page 1354
    Author:
    Ushimaru, Shinji
    ,
    Tanaka, Hiroshi
    DOI: 10.1175/1520-0469(1992)049<1354:ANSOTI>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Quasi-stationary Rossby waves with a wavenumber 1 component (wave 1) and eastward-traveling waves with a wavenumber 2 component (wave 2), whose period lies in 10?20 days, have been frequently observed during the late winter and early spring in the stratosphere of the Southern Hemisphere. Temporal variations of these amplitudes are remarkably enhanced during this period.The interaction among wave 1, wave 2, and the zonal mean flow was simulated using a low-order truncated semispectral model. It was assumed that both the stationary wave 1 and eastward-traveling wave 2 are forced at the tropopause. When the wavenumbers from 1 to 3 or 4 were included in the model with use of a reasonable forcing amplitude and the observed monthly mean zonal wind, the following results were obtained. 1) The amplitude of wave 1 reaches a maximum value when the ridge of wave 2 overlaps that of wave 1. 2) The amplitude of wave 2 is negatively correlated with wave 1. 3) In many cases the large amplification of wave 1 occurs only once for every two passages of wave 2 over wave 1.From the analysis of energetics, it was found that the amplification of wave 1 arises from the abrupt decrease of kinetic energy conversion to the zonal mean flow. The analysis of potential enstrophy conversion revealed more clearly that the amplification of wave 1 is caused by the wave-mean flow interaction. Eliassen-Palm (E?P) flux of wave 1 focuses to the high-latitude stratosphere during the amplification stage. The focusing is caused by appearance of the negative refractive index for wave 1 in the midlatitudes, that is, formation of waveguide in the high latitudes.The interaction between wave 1 and wave 2 causes the periodic variation of wave amplitudes through their energy/enstrophy exchange and controls degree of the interaction with zonal mean flow through the horizontal phase movement. In the amplification stage, the wave-wave interaction emphasizes the focus of E?P flux.
    • Download: (1.557Mb)
    • Show Full MetaData Hide Full MetaData
    • Item Order
    • Go To Publisher
    • Price: 5000 Rial
    • Statistics

      A Numerical Study of the Interaction between Stationary Rossby Waves and Eastward-Traveling Waves in the Southern Hemisphere Stratosphere

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4156988
    Collections
    • Journal of the Atmospheric Sciences

    Show full item record

    contributor authorUshimaru, Shinji
    contributor authorTanaka, Hiroshi
    date accessioned2017-06-09T14:30:56Z
    date available2017-06-09T14:30:56Z
    date copyright1992/08/01
    date issued1992
    identifier issn0022-4928
    identifier otherams-20728.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156988
    description abstractQuasi-stationary Rossby waves with a wavenumber 1 component (wave 1) and eastward-traveling waves with a wavenumber 2 component (wave 2), whose period lies in 10?20 days, have been frequently observed during the late winter and early spring in the stratosphere of the Southern Hemisphere. Temporal variations of these amplitudes are remarkably enhanced during this period.The interaction among wave 1, wave 2, and the zonal mean flow was simulated using a low-order truncated semispectral model. It was assumed that both the stationary wave 1 and eastward-traveling wave 2 are forced at the tropopause. When the wavenumbers from 1 to 3 or 4 were included in the model with use of a reasonable forcing amplitude and the observed monthly mean zonal wind, the following results were obtained. 1) The amplitude of wave 1 reaches a maximum value when the ridge of wave 2 overlaps that of wave 1. 2) The amplitude of wave 2 is negatively correlated with wave 1. 3) In many cases the large amplification of wave 1 occurs only once for every two passages of wave 2 over wave 1.From the analysis of energetics, it was found that the amplification of wave 1 arises from the abrupt decrease of kinetic energy conversion to the zonal mean flow. The analysis of potential enstrophy conversion revealed more clearly that the amplification of wave 1 is caused by the wave-mean flow interaction. Eliassen-Palm (E?P) flux of wave 1 focuses to the high-latitude stratosphere during the amplification stage. The focusing is caused by appearance of the negative refractive index for wave 1 in the midlatitudes, that is, formation of waveguide in the high latitudes.The interaction between wave 1 and wave 2 causes the periodic variation of wave amplitudes through their energy/enstrophy exchange and controls degree of the interaction with zonal mean flow through the horizontal phase movement. In the amplification stage, the wave-wave interaction emphasizes the focus of E?P flux.
    publisherAmerican Meteorological Society
    titleA Numerical Study of the Interaction between Stationary Rossby Waves and Eastward-Traveling Waves in the Southern Hemisphere Stratosphere
    typeJournal Paper
    journal volume49
    journal issue15
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1992)049<1354:ANSOTI>2.0.CO;2
    journal fristpage1354
    journal lastpage1373
    treeJournal of the Atmospheric Sciences:;1992:;Volume( 049 ):;issue: 015
    contenttypeFulltext
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian
     
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian