Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4388
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dc.contributor.authorBanerjee, D-
dc.contributor.authorHasan, S. S-
dc.contributor.authorChristensen-Dalsgaard, J-
dc.date.accessioned2009-03-05T16:30:01Z-
dc.date.available2009-03-05T16:30:01Z-
dc.date.issued1997-
dc.identifier.citationF.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 - 280en
dc.identifier.isbn0-7923-4902-4-
dc.identifier.urihttp://hdl.handle.net/2248/4388-
dc.descriptionRestricted Access-
dc.description.abstractWe 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.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.ispartofseriesAstrophysics and Space Science Library, Vol. 225-
dc.relation.urihttp://adsabs.harvard.edu/abs/1997ASSL..225..277Ben
dc.subjectSolar Physics-
dc.subjectMHD-
dc.subjectMagnetic Fields-
dc.subjectOscillations-
dc.titleThe influence of radiative damping on the modes of a magnetized isothermal atmosphereen
dc.typeArticleen
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