Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3772
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dc.contributor.authorJoarder, P. S-
dc.contributor.authorGokhale, M. H-
dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-09-22T12:27:26Z-
dc.date.available2008-09-22T12:27:26Z-
dc.date.issued1987-09-
dc.identifier.citationSolar Physics , Vol. 110, No. 2, pp. 255 - 270en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/3772-
dc.description.abstractThe authors investigate the effects of radiative heat losses and thermal conductivity on the hydromagnetic surface waves along a magnetic discontinuity in a plasma of infinite electrical conductivity. They show that the effects of radiative heat losses on such surface waves are appreciable only when values of the plasma pressure on the two sides of the discontinuity are substantially different. Overstability of a surface wave requires that the medium in which it gives larger first-order compression should satisfy the criterion of Field (1965). Possible applications of the study to magnetic discontinuities in solar corona are briefly discussed.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1007/BF00206422en
dc.subjectMagnetohydrodynamic wavesen
dc.subjectPlasma conductivityen
dc.subjectPlasma densityen
dc.subjectRadiative heat transferen
dc.subjectSurface wavesen
dc.subjectThermal stabilityen
dc.subjectPlasma compressionen
dc.subjectPlasma pressureen
dc.subjectSolar coronaen
dc.subjectSolar magnetic fielden
dc.titleThermal overstability of hydromagnetic surface wavesen
dc.typeArticleen
Appears in Collections:IIAP Publications

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