Abstract
An analytical spectral model of the barotropic divergent equations on a sphere is developed using the potential-stream function formulation and the normal modes as basic functions. Explicit expressions of the coefficients of nonlinear interaction are obtained in the asymptotic case of a slowly rotating sphere, i.e. when the normal modes can be expressed as single spherical harmonics.
Highly truncated versions of the model are used to illustrate some consequences of the interaction between the Rossby waves and the surface gravity waves. So, it is shown how the gravity waves can exchange energy through interaction with a Rossby wave. A particular interaction between a Rossby wave and a gravity wave of zonal wavenumbers m and 2m, respectively, is discussed in greater detail and is shown to lead to a frequency shift of the Rossby wave.
The stability of the Rossby waves to perturbations involving one or two gravity waves is examined and it is shown that the corresponding critical amplitudes are unrealistically large. The decay of the Rossby waves will probably be governed by the interactions inside Rossby waves triads.
| Original language | English |
|---|---|
| Pages (from-to) | 121-144 |
| Number of pages | 24 |
| Journal | Geophysical and astrophysical fluid dynamics |
| Volume | 76 |
| Issue number | 1-4 |
| Publication status | Published - 1994 |
Keywords / Materials (for Non-textual outputs)
- ROSSBY WAVES
- GRAVITY WAVES
- NONLINEAR INTERACTIONS
- WAVE INSTABILITY
- BAROTROPIC PRIMITIVE EQUATIONS
- HOUGH HARMONIC EXPANSIONS
- PLANETARY-WAVES
- MODEL