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Issue A&A
Volume 451, Number 1, May III 2006
Page(s) 273 - 284
Section Stellar atmospheres
DOI http://dx.doi.org/10.1051/0004-6361:20053846

A&A 451, 273-284 (2006)
DOI: 10.1051/0004-6361:20053846

A 3D radiative transfer framework

I. Non-local operator splitting and continuum scattering problems
P. H. Hauschildt1 and E. Baron1, 2, 3

1  Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany
    e-mail: yeti@hs.uni-hamburg.de
2  Homer L. Dodge Dept. of Physics and Astronomy, University of Oklahoma, 440 W. Brooks, Rm 100, Norman, OK 73019-2061, USA
    e-mail: baron@nhn.ou.edu
3  CRD, Lawrence Berkeley National Laboratory, MS 50F-1650, 1 Cyclotron Rd, Berkeley, CA 94720-8139, USA

(Received 18 July 2005 / Accepted 3 January 2006)

Abstract
We describe a highly flexible framework to solve 3D radiation transfer problems in scattering dominated environments based on a long characteristics piece-wise parabolic formal solution and an operator splitting method. We find that the linear systems are efficiently solved with iterative solvers such as Gauss-Seidel and Jordan techniques. We use a sphere-in-a-box test model to compare the 3D results to 1D solutions in order to assess the accuracy of the method. We have implemented the method for static media, however, it can be used to solve problems in the Eulerian-frame for media with low velocity fields.


Key words: radiative transfer





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