Gravitational Signature of Jupiter's Deep Zonal Flows
โ Scribed by W.B. Hubbard
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 65 KB
- Volume
- 137
- Category
- Article
- ISSN
- 0019-1035
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๐ SIMILAR VOLUMES
Measurements from the Galileo probe suggest that the zonal winds are deep rooted. Jupiter's high rotation rate makes it likely that the whole outer molecular H/He layer is involved in these longlived jet flows. Assuming that the primary flows are geostrophic, and that the banded surface structure st
The initial development of an anticyclonic eddy in a high-speed jet flow has been examined using a two-layer rigid-lid model for incompressible fluid governed by the shallow water equations. In the case of large Rossby deformation radius an inertia-gravity wave can propagate in all directions, but i