Comments on Viscous Damping of Non-Adiabatic MHD Waves in an Unbounded Solar Coronal Plasma by Kumar and Kumar

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dc.creatorPandey, V. S.
dc.creatorDwivedi, B. N.
dc.date2006-11-08
dc.date2007-06-22
dc.date.accessioned2026-07-07T08:11:36Z
dc.date.available2026-07-07T08:11:36Z
dc.descriptionConsidering thermal conduction, compressive viscosity and optically thin radiation as damping mechanisms for MHD waves, we derive a six-order general dispersion relation. We point out a fundamental flaw in the derivation of five-order dispersion relation by Kumar and Kumar (2006) who adopt as a basis vector. The correct definition of the motion in the x-z plane (2-D vector space) stems from the two independent variables, namely .
dc.description8 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0611252
dc.identifierhttp://arxiv.org/abs/astro-ph/0611252
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132169
dc.subjectAstrophysics
dc.titleComments on Viscous Damping of Non-Adiabatic MHD Waves in an Unbounded Solar Coronal Plasma by Kumar and Kumar
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