FINITE-AMPLITUDE THREE-DIMENSIONAL HARMONIC WAVES ON THE SPHERICAL EARTH
- 1 October 1959
- journal article
- Published by American Meteorological Society in Journal of Meteorology
- Vol. 16 (5) , 524-534
- https://doi.org/10.1175/1520-0469(1959)016<0524:fatdhw>2.0.co;2
Abstract
By making use of the quasi-nondivergent approximation, the potential vorticity equation is reduced to an equation in the stream function ψ. Assuming that the motion is of permanent wave type, a first integral of this nonlinear vorticity equation is obtained, which itself is a linear three-dimensional partial differential equation in ψ. This equation has been solved as a boundary-value problem by the method of separation of variables. It is found that the latitudinal-amplitude functions of these waves satisfy a spheroidal-wave equation while the vertical-amplitude functions are given by Bessel and Hankel functions of the argument lp/p0, where l is a parameter depending on both the static stability and the nodal number r. The eigenvalues µmr of these wave solutions are connected with the parameter l2 by a transcendental relation. We have expanded µmr into a power series of l2 and obtained the various coefficients, up to that of the fourth power of l2. The latitudinal- and vertical-amplitude functio... Abstract By making use of the quasi-nondivergent approximation, the potential vorticity equation is reduced to an equation in the stream function ψ. Assuming that the motion is of permanent wave type, a first integral of this nonlinear vorticity equation is obtained, which itself is a linear three-dimensional partial differential equation in ψ. This equation has been solved as a boundary-value problem by the method of separation of variables. It is found that the latitudinal-amplitude functions of these waves satisfy a spheroidal-wave equation while the vertical-amplitude functions are given by Bessel and Hankel functions of the argument lp/p0, where l is a parameter depending on both the static stability and the nodal number r. The eigenvalues µmr of these wave solutions are connected with the parameter l2 by a transcendental relation. We have expanded µmr into a power series of l2 and obtained the various coefficients, up to that of the fourth power of l2. The latitudinal- and vertical-amplitude functio...Keywords
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