Overstable Convective Modes in a Polytropic Stellar Atmosphere
Within the convection zone of a rotating star, the presence of the Coriolis force stabilizes long-wavelength convective modes. These modes, which would have been unstable if the star lacked rotation, are called overstable convective modes or thermal Rossby waves. We demonstrate that the Sun’s rotati...
| Auteurs principaux: | , |
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| Format: | Article |
| Langue: | English |
| Publié: |
IOP Publishing
2023-01-01
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| Collection: | The Astrophysical Journal |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.3847/1538-4357/acaec4 |