Abstract
We have developed a computer program, Multi3D, for solving non-LTE radiative transfer problems in three dimensional geometry. Boundaries can be periodic or the radiation field may be prescribed. The atomic model may contain many energy levels. A short characteristic method is used for the radiative transfer and the rate equations are linearized such that a generalization to radiation hydrodynamics is straightforward. The code can be run on parallel computer architectures using MPI. The parallel speed-up is linear up to the number of nodes equal to the number of bound-bound transitions in the atom. Examples are given for the formation of the resonance lines of neutral sodium, Nal D, and singly ionized calcium, Call K, in a simulation of the solar convection using 3, 6 and 12 level model atoms and 32 x 32 x 100 points in the atmosphere.
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References
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© 1999 Springer Science+Business Media Dordrecht
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Botnen, A., Carlsson, M. (1999). Multi3D, 3D Non-Lte Radiative Transfer. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_113
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DOI: https://doi.org/10.1007/978-94-011-4780-4_113
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6008-0
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