Stability of solar protuberances
This method of stability analysis was developed for stellar envelopes and it is extended to solar protuberances taking into account the boundary conditions of this case. This is a first approximation to the study of the stability of solar protuberances because this chemical compositions have been si...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1987
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/137632 |
| Aporte de: |
| Sumario: | This method of stability analysis was developed for stellar envelopes and it is extended to solar protuberances taking into account the boundary conditions of this case. This is a first approximation to the study of the stability of solar protuberances because this chemical compositions have been simplified. Only hydrogen in its fundamental state and ionized hydrogen have been considered. In the optically thick case, the instability depends on the incident radiation coming from the photosphere and chromosphere. |
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