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The influence of radiative damping on the modes of a magnetized isothermal atmosphere

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dc.contributor.author Banerjee, D
dc.contributor.author Hasan, S. S
dc.contributor.author Christensen-Dalsgaard, J
dc.date.accessioned 2009-03-05T16:30:01Z
dc.date.available 2009-03-05T16:30:01Z
dc.date.issued 1997
dc.identifier.citation F.P. Pijpers, J. Christensen-Dalsgaard, and C.S. Rosenthal., eds., SCORe'96 : Solar Convection and Oscillations and their Relationship, Proceedings of a workshop, held in Aarhus, Denmark, May 27 - 31, 1996, pp. 277 - 280 en
dc.identifier.isbn 0-7923-4902-4
dc.identifier.uri http://hdl.handle.net/2248/4388
dc.description Restricted Access
dc.description.abstract We examine the influence of radiative damping on the modes of an isothermal magnetized plasma. This investigation is an extension of earlier work by Hasan & Christensen-Dalsgaard (1992) and Banerjee, Hasan & Christensen-Dalsgaard (1995, 1996), which treated the effects of a uniform vertical magnetic field on the adiabatic modes of a stratified atmosphere. We focus on the properties of the Lamb mode and examine its interaction with a magnetic mode. We show that radiative dissipation can significantly alter the Lamb-mode frequency and lead to a enhanced damping of the waves at the avoided crossings in the k - w diagram. This mechanism could be important for wave damping in flux tubes on the Sun.
dc.language.iso en en
dc.publisher Kluwer Academic Publishers en
dc.relation.ispartofseries Astrophysics and Space Science Library, Vol. 225
dc.relation.uri http://adsabs.harvard.edu/abs/1997ASSL..225..277B en
dc.subject Solar Physics
dc.subject MHD
dc.subject Magnetic Fields
dc.subject Oscillations
dc.title The influence of radiative damping on the modes of a magnetized isothermal atmosphere en
dc.type Article en


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