pure and applied geophysics

, Volume 157, Issue 10, pp 1767–1779 | Cite as

Equatorial Meridional Flows: Rotationally Induced Circulations

  • W. H. Raymond


—This study examines two-dimensional large-scale atmospheric circulations that are centered over the equator. The influence of terms that contain the Coriolis parameter ƒ′=2ΩcosΘ is highlighted in a simple linear inviscid equatorial beta model. Two general types of oscillatory circulations are identified within the yz plane. In a neutral or stably stratified atmosphere one circulation is expressed in terms of an analytic solution that contains Hermite polynomials, while a second solution is described in terms of a Bessel function. In the more traditional Hermite polynomial solution the influence of f′ is small as suggested by scale analysis. Neutral stability provides the only exception. In contrast to these findings, the Bessel solution contains frequencies with semiannual periods that depend entirely on ƒ′≠0. This solution describes cross-equatorial flow with a maximum meridional velocity at the equator. Consequently, this indicates that to model the atmosphere it is necessary to include in the model equations all terms containing f′, since they influence oscillatory circulations that describe internal waves with periods that vary from a few days to semiannual.

Key Words: Meridional flow, Coriolis parameters, equatorial flow, oscillations, analytic solutions, y – z plane. 


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Copyright information

© Birkhäuser Verlag Basel, 2000

Authors and Affiliations

  • W. H. Raymond
    • 1
  1. 1.Cooperative Institute for Meteorological Satellite Studies, University of Wisconsin, 1225 West Dayton Street, Madison, Wisconsin 53706, U.S.A. E-mail: wraymond@mail.ssec.wisc.edu Telefacsimile: 608 2625974.US

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