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Quasi-Geostrophic Modes (Rossby Waves)

For f = constant, (3.2) can be satisfied for arbitrary tex2html_wrap_inline5879 if tex2html_wrap_inline5133 = 0, in which case (3.1) reduces to an exact geostrophic balance tex2html_wrap_inline6053 where

displaymath6055

In fact, for the real world, f depends upon latitude tex2html_wrap_inline6059 and hence

displaymath6061

which vanishes only if tex2html_wrap_inline5879 is a function of latitude (implying zonal geostrophic flow). Thus if the flow (even though nearly geostrophic) has a component across the contours of f (meridional component), then the field of tex2html_wrap_inline5879 must change with time (see Eq. 2.12).

The possibility of wave modes with very small frequency as solutions of the LTEs was first recognized by Laplace, who termed these ``waves of the second class.'' They differ from the gravity wave counterparts in that they have large vorticity relative to horizontal divergence. For this reason a logical generic name is vortex modes; although from the standpoint of restoring ``force'' they are sometimes called inertial modes, since gravity plays only a secondary role.

Although one can derive both the gravity wave modes and the vortex modes simultaneously form the LTEs with allowance for variable f, a much simpler analysis of the vortex mode properties follows from the quasigeostrophic vorticity equation, as first recognized by Carl-G. Rossby (1936, J. Mar. Res.). We give a generalization of this methodology here. It is for reasons of the recognition of this methodology that the vortex modes are so commonly called Rossby waves. He was the first to recognize their importance in the dynamics of the ocean and the atmosphere.




next up previous contents
Next: The Quasi-Geostrophic Vorticity Equation Up: Very Low Frequency Waves Previous: Gravity Modes for f

Steve Baum
Sun May 19 00:59:05 CDT 1996