Numerical simulation of the cooling of a solar flare

Numerical simulation of the cooling of a solar flare

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Se usa un código hidrodinámico unidimensional para estudiar el enfriamiento de destellos solares. El enfriamiento del flujo a través del tubo magnético se calcula para el caso en el cual la atmósfera se encuentra inicialmente en equilibrio térmico con una temperatura máxima de 107 K. A medida que el...

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Bibliographic Details
Main Authors:	César A. Mendoza-Briceño, Leonardo Sigalotti, Neyda Y. Añez-Parra
Format:	Article
Language:	English
Published:	Universidad Nacional Autónoma de México, Instituto de Geofísica 2004-01-01
Series:	Geofísica Internacional
Subjects:	destello solar atmósfera solar hidrodinámica
Online Access:	http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/925

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