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Please use this identifier to cite or link to this item: https://doi.org/10.1007/BF00651020
DC FieldValue
dc.titleLocal potential analysis of MHD instability
dc.contributor.authorSen, K.K.
dc.contributor.authorWilson, S.J.
dc.date.accessioned2014-10-28T02:38:11Z
dc.date.available2014-10-28T02:38:11Z
dc.date.issued1985-02
dc.identifier.citationSen, 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
dc.identifier.issn0004640X
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/103514
dc.description.abstractIn 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.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1007/BF00651020
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentMATHEMATICS
dc.description.doi10.1007/BF00651020
dc.description.sourcetitleAstrophysics and Space Science
dc.description.volume109
dc.description.issue1
dc.description.page131-143
dc.identifier.isiutA1985ADL4400011
Appears in Collections:Staff Publications

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