Analysis of a model in solar magnetohydrostatics

The model for resistive diffusion of a force-free magnetic field in a compressible plasma is analysed. Such a model has been suggested for describing the behavior of the solar outer atmosphere and that of solar flares. Previous analysis of the model involved assumptions of linear plasma velocity and...

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Bibliographic Details
Main Author: David Eberly
Format: Article
Language:English
Published: Wiley 1990-01-01
Series:International Journal of Mathematics and Mathematical Sciences
Subjects:
Online Access:http://dx.doi.org/10.1155/S0161171290001041
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