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On general transformations and variational Principles of an ideal three-dimensional compressible

Published online by Cambridge University Press:  01 November 2006

A. H. Khater ,
D. K. Callebaut  and
T. N. Abdelhameed
A. H. Khater
Affiliation:
Department of Mathematics, Faculty of Science, Beni-Suef University, Beni-Suef, Egypt email: khater_ah@yahoo.com & tarknabil_1312000@yahoo.com Department Natuurkunde, CGB, University of Antwerp, B-2020 Antwerp, Belgium email: dirk.callebaut@ua.ac.be
D. K. Callebaut
Affiliation:
Department Natuurkunde, CGB, University of Antwerp, B-2020 Antwerp, Belgium email: dirk.callebaut@ua.ac.be
T. N. Abdelhameed
Affiliation:
Department of Mathematics, Faculty of Science, Beni-Suef University, Beni-Suef, Egypt email: khater_ah@yahoo.com & tarknabil_1312000@yahoo.com
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Abstract

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In this paper we have used the general theory of Arnold (1965,1966) and Vladimirov et al. (1997) to obtain sufficient conditions for linear stability of steady MHD flows of an ideal three-dimensional compressible gravitating flows.

Keywords

magnetohydrodynamicsgravitating fluidstability
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 304 - 306
Copyright
© 2006 International Astronomical Union