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40 - Vertical motion in the monsoon circulation

Published online by Cambridge University Press:  05 November 2011

M. C. Sinha
Affiliation:
India Meteorology Department
O. P. Sharma
Affiliation:
India Meteorological Department
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Summary

A review is presented of methods for solving the omega-equation by (a) finite differences, and (b) finite elements. The different types of forcing terms that arise when the wind vector is resolved into a rotational and a solenoidal part are described. A computational procedure for evaluating omega by successive approximations is outlined. Computations of omega by the method of finite elements, using prismatic elements, is described. Results of omega computations made by finite differences and by finite elements are presented and discussed.

Introduction

A problem of considerable importance in meteorology is the estimation of vertical velocity. As its magnitude is very small, direct measurements are not possible. Consequently, the pattern of vertical velocity is usually inferred from measurements of horizontal velocity, the pressure and temperature distribution in the atmosphere. A commonly used technique is to derive a solution of the diagnostic omega-equation. An excellent review of vertical velociy computations has been provided by Pearce (1974). In this paper we wish to consider solutions of the omega-equation by (a) finite differences, and (b) by the method of finite elements.

Basic equations

The basic equations express the first law of thermodynamics, the conservation of vorticity and conservation of mass. Pressure coordinates are generally used to derive the omega-equation but, as we shall see later, this gives rise to difficulties in the vicinity of steep orographic features.

Type
Chapter
Information
Monsoon Dynamics , pp. 601 - 614
Publisher: Cambridge University Press
Print publication year: 1981

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