Please use this identifier to cite or link to this item:
|Title:||Local potential analysis of MHD instability||Authors:||Sen, K.K.
|Issue Date:||Feb-1985||Citation:||Sen, K.K., Wilson, S.J. (1985-02). Local potential analysis of MHD instability. Astrophysics and Space Science 109 (1) : 131-143. ScholarBank@NUS Repository. https://doi.org/10.1007/BF00651020||Abstract:||In many astrophysical problems, the study of the stability of an atmosphere in the presence of a magnetic field is of importance. In most cases the MHD instabilities of atmospheres are studied by energy principle of Bernstein et al. (1958). In this paper, a general method for studying the stability of a system subject to MHD equations of conditions has been proposed. This is based on the local potential concept put forward by Glansdorff and Prigogine (1964). The scheme for securing stability criteria has been demonstrated in two particular cases. © 1985 D. Reidel Publishing Company.||Source Title:||Astrophysics and Space Science||URI:||http://scholarbank.nus.edu.sg/handle/10635/103514||ISSN:||0004640X||DOI:||10.1007/BF00651020|
|Appears in Collections:||Staff Publications|
Show full item record
Files in This Item:
There are no files associated with this item.
checked on Jun 23, 2022
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.