Wave propagation in the magnetic sun

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This 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.
6 pages

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/160268

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0805.0333
 http://arxiv.org/abs/0805.0333
 Proceedings of the 2006 Summer Program, Center for Turbulence Research, Stanford/NASA Ames Research Center, pp. 399-404

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arXiv