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...

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Autores principales: Hernaiz, A.F., Fontenla, J.M.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1987
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/137632
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id I19-R120-10915-137632
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Hernaiz, A.F.
Fontenla, J.M.
Stability of solar protuberances
topic_facet Astronomía
Galaxias
description 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.
format Articulo
Comunicacion
author Hernaiz, A.F.
Fontenla, J.M.
author_facet Hernaiz, A.F.
Fontenla, J.M.
author_sort Hernaiz, A.F.
title Stability of solar protuberances
title_short Stability of solar protuberances
title_full Stability of solar protuberances
title_fullStr Stability of solar protuberances
title_full_unstemmed Stability of solar protuberances
title_sort stability of solar protuberances
publishDate 1987
url http://sedici.unlp.edu.ar/handle/10915/137632
work_keys_str_mv AT hernaizaf stabilityofsolarprotuberances
AT fontenlajm stabilityofsolarprotuberances
bdutipo_str Repositorios
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