Four Numerical Approaches for Solving the Radiative Transfer Equation in Magnetized White-Dwarf Atmospheres

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dc.creatorJordan, Stefan
dc.creatorSchmidt, Holger
dc.date2003-02-04
dc.date.accessioned2026-07-07T02:07:28Z
dc.date.available2026-07-07T02:07:28Z
dc.descriptionWe compare four different methods to calculate radiative transfer through a magnetized stellar atmosphere, and apply them to the case of magnetic white dwarfs. All methods are numerically stable enough to allow determination of the magnetic field structure, but distinctions between faster, simplifying, methods, and elaborate, but more CPU-time consuming, methods, can be made.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0302047
dc.identifierhttp://arxiv.org/abs/astro-ph/0302047
dc.identifierASP conference series, Workshop on Atmosphere Modeling, Tuebingen, April 8-12, 2002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5703
dc.subjectAstrophysics
dc.titleFour Numerical Approaches for Solving the Radiative Transfer Equation in Magnetized White-Dwarf Atmospheres
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