Evolution of the fluid models for the solar coronal expansion

Autores/as

  • Alexander P. Departamento de Física, Facultad de Ciencias Exactas y Naturales Universidad de Buenos Aires

Resumen

El interrogante acerca de cómo la corona solar se expande hacia la región interplanetaria circundante ha sido uno de los temas más apasionantes de la ciencia espacial desde fines de la década del '50 y está aún lejos de una respuesta definitiva. El presente escrito hace una revisión de las observaciones y teorías que condujeron al concepto de esa expansión y describe los modelos subsiguientes hasta la actualidad. Finalmente se mencionan algunos de los interrogantes abiertos de este fenómeno.

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Publicado

1993-12-12

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P., A. (1993). Evolution of the fluid models for the solar coronal expansion. Geoacta, 20, 1–10. Recuperado a partir de https://revistas.unlp.edu.ar/geoacta/article/view/13696

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