Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3792
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dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-09-22T16:49:44Z-
dc.date.available2008-09-22T16:49:44Z-
dc.date.issued1985-03-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 6, No. 1, pp. 21 - 34en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3792-
dc.description.abstractInclusion of radiative heat transport in the energy equation for a slender flux tube leads to oscillations of the tube. The amplitude of the oscillations depends on the radius of the tube when lateral heat exchange alone is considered. Longitudinal heat transport has a greater influence on the evolution of the instability than lateral heat exchange for the particular value of tube radius considered in the calculation. Heat transport is seen to reduce the efficiency of concentration of magnetic fields by convective collapse in the case of polytropic tubes.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1985JApA....6...21Ven
dc.subjectConvectionen
dc.subjectMagnetohydrodynamic Stabilityen
dc.subjectRadiative Heat Transferen
dc.subjectSolar Magnetic Fielden
dc.subjectBoundary Value Problemsen
dc.subjectMagnetic Fluxen
dc.subjectTemperature Gradientsen
dc.subjectThermal Conductivityen
dc.subjectThermal Conductivityen
dc.subjectUnsteady Flowen
dc.subjectVelocity Distributionen
dc.titleNonlinear development of convective instability within slender flux tubes. II - The effect of radiative heat transporten
dc.typeArticleen
Appears in Collections:IIAP Publications

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