Parker’s Solar Wind Model for a Polytropic Gas
Parker’s hydrodynamic isothermal solar wind model is extended to apply for a more realistic polytropic gas flow that can be caused by a variable extended heating of the corona. A compatible theoretical formulation is given and detailed numerical and systematic asymptotic theoretical considerations a...
Guardado en:
Autores principales: | Bhimsen Shivamoggi, David Rollins, Leos Pohl |
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Formato: | article |
Lenguaje: | EN |
Publicado: |
MDPI AG
2021
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Materias: | |
Acceso en línea: | https://doaj.org/article/809e092da57e42dfab1f714a566cbcd3 |
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