The Propagation of Flare Generated Shockwaves in Self-Gravitating Solar Atmosphere

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Published: 2013-09-15
Keywords:
Shockwaves, Solar Atmosphere, Fundamental equation for spherically symmetric flow of a self graviting atmosphere in the presence of magnetic field.

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S. N. Ojha
Department of Mathematics, S. C. College Ballia (U.P.)
Awaneesh Jee Srivastava
S. R. M. G. P. C., Lucknow (U.P.)

Abstract

The effects of an interplanetary magnetic field on the
propagation of the flare generated shock wave in a non-uniformly
distributed solar self-gravitating atmosphere are investigated by using
an approximate analytic method of Whitham. The expressions for the
velocity of shock wave and for the other flow variables behind weak
and strong shocks are derived and discussed.

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Vol. 17 No. 3 (2013): Table of Content

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Articles
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This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.

How to Cite

1.
The Propagation of Flare Generated Shockwaves in Self-Gravitating Solar Atmosphere. J. Int. Acad. Phys. Sci. [Internet]. 2013 Sep. 15 [cited 2026 Oct. 23];17(3):223-32. Available from: http://www.iaps.org.in/journal/index.php/journaliaps/article/view/548

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