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Characterization of columnar inertial modes in rapidly rotating spheres and spheroids
We consider fluid-filled spheres and spheroidal containers of eccentricity ϵ in rapid rotation, as a proxy for the interior dynamics of stars and planets. The fluid motion is assumed to be quasi-geostrophic (QG): horizontal motions are invariant parallel to the rotation axis z, a characteristic whic...
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| Publicado en: | Proc Math Phys Eng Sci |
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| Autores principales: | , , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
The Royal Society Publishing
2017
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| Materias: | |
| Acceso en línea: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5582179/ https://ncbi.nlm.nih.gov/pubmed/28878558 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rspa.2017.0181 |
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