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    Observational Study of the Tropical Upper Tropospheric Motion Field during the Northern Hemisphere Summer

    Source: Journal of Applied Meteorology:;1971:;volume( 010 ):;issue: 006::page 1066
    Author:
    Krishnamurti, T. N.
    DOI: 10.1175/1520-0450(1971)010<1066:OSOTTU>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Conventional and commerical aircraft wind observations over the global tropics have been used to prepare daily charts of the field of motion at the 200-mb level for June, July and August 1967. Computations describe the climatology of the field of motion (streamlies and isotachs) and the divergence and vorticity distributions. A number of dynamical computations are made utilizing these data. These include 1) A comparison of the strength of the rotational part of the wind with the total wind. 2) A description of the strength and geometry of the Hadley and Walker circulations. 3) An analysis of the ultralong waves (zonal wavenumbers 1 and 2). The waves, which are quasi-stationary, are shown to carry a large proportion of the total variance of the motion field and to have a very pronounced southwest to northeast tilt. The amplitude and motion of transient ultralong waves, wavenumbers 1 and 2, are studied on polar diagrams. It is shown that these waves are intermittent and rapidly moving. 4) An analysis of the amplitude and motion of shorter waves (wavenumbers 7 and 8 of the zonal spectra of the meridional wind), which are intermittent, have been studied on x?t diagrams. Their amplitudes and speeds of westward propagation vary respectively between 0 and 6 m sec?1 and 4° to 12° longitude day?1. 5) A computation of the energy exchange between the zonal flow and eddies. Quasi-periodic oscillations in time are shown with a period of roughly 3.5 days. The phenomenon is suggested to be a manifestation of pure barotropic type instability of the tropical upper level flows. 6) Computations of meridional fluxes of momentum and kinetic energy. These are shown to be related to the shapes of the quasi-stationery ultralong waves and possibly also to certain shapes of westward moving shorter waves over the Northern Hemisphere tropics.
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      Observational Study of the Tropical Upper Tropospheric Motion Field during the Northern Hemisphere Summer

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4225600
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    contributor authorKrishnamurti, T. N.
    date accessioned2017-06-09T17:17:24Z
    date available2017-06-09T17:17:24Z
    date copyright1971/12/01
    date issued1971
    identifier issn0021-8952
    identifier otherams-8248.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4225600
    description abstractConventional and commerical aircraft wind observations over the global tropics have been used to prepare daily charts of the field of motion at the 200-mb level for June, July and August 1967. Computations describe the climatology of the field of motion (streamlies and isotachs) and the divergence and vorticity distributions. A number of dynamical computations are made utilizing these data. These include 1) A comparison of the strength of the rotational part of the wind with the total wind. 2) A description of the strength and geometry of the Hadley and Walker circulations. 3) An analysis of the ultralong waves (zonal wavenumbers 1 and 2). The waves, which are quasi-stationary, are shown to carry a large proportion of the total variance of the motion field and to have a very pronounced southwest to northeast tilt. The amplitude and motion of transient ultralong waves, wavenumbers 1 and 2, are studied on polar diagrams. It is shown that these waves are intermittent and rapidly moving. 4) An analysis of the amplitude and motion of shorter waves (wavenumbers 7 and 8 of the zonal spectra of the meridional wind), which are intermittent, have been studied on x?t diagrams. Their amplitudes and speeds of westward propagation vary respectively between 0 and 6 m sec?1 and 4° to 12° longitude day?1. 5) A computation of the energy exchange between the zonal flow and eddies. Quasi-periodic oscillations in time are shown with a period of roughly 3.5 days. The phenomenon is suggested to be a manifestation of pure barotropic type instability of the tropical upper level flows. 6) Computations of meridional fluxes of momentum and kinetic energy. These are shown to be related to the shapes of the quasi-stationery ultralong waves and possibly also to certain shapes of westward moving shorter waves over the Northern Hemisphere tropics.
    publisherAmerican Meteorological Society
    titleObservational Study of the Tropical Upper Tropospheric Motion Field during the Northern Hemisphere Summer
    typeJournal Paper
    journal volume10
    journal issue6
    journal titleJournal of Applied Meteorology
    identifier doi10.1175/1520-0450(1971)010<1066:OSOTTU>2.0.CO;2
    journal fristpage1066
    journal lastpage1096
    treeJournal of Applied Meteorology:;1971:;volume( 010 ):;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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