Abstract
The intrinsic westward drift of oceanic monopolar vortices is explained in terms of angular momentum dynamics. In turn, the physical origin of this is shown to reside in the broken spherical symmetry of the fluid dynamics on a rotating planet. This is done developing and applying a slight generalization of Noether's theorem. As a preliminary, the gravitational field of a rotating planet is analyzed in detail.
Original language | English |
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Awarding Institution |
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Award date | 1 Oct 1997 |
Print ISBNs | 90-393-1602-3 |
Electronic ISBNs | 9789039316023 |
Publication status | Published - 1 Oct 1997 |
Externally published | Yes |
Keywords
- planetary fluid dynamics
- planetary gravitation
- monopolar vortices
- angular momentum dynamics
- variational principle
- Lie algebra
- rotational symmetry