Wave propagation in the magnetic sun

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dc.creatorHartlep, T.
dc.creatorMiesch, M. S.
dc.creatorMansour, N. N.
dc.date2008-05-03
dc.date.accessioned2026-07-07T09:36:52Z
dc.date.available2026-07-07T09:36:52Z
dc.descriptionThis paper reports on efforts to simulate wave propagation in the solar interior. Presented is work on extending a numerical code for constant entropy acoustic waves in the absence of magnetic fields to the case where magnetic fields are present. A set of linearized magnetohydrodynamic (MHD) perturbation equations has been derived and implemented.
dc.description6 pages
dc.identifierhttps://arxiv.org/abs/0805.0333
dc.identifierhttp://arxiv.org/abs/0805.0333
dc.identifierProceedings of the 2006 Summer Program, Center for Turbulence Research, Stanford/NASA Ames Research Center, pp. 399-404
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160268
dc.subjectAstrophysics
dc.titleWave propagation in the magnetic sun
dc.typetext

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