EAS Publications Series
Volume 18, 2006Radiative Transfer and Applications to Very Large Telescopes
|Page(s)||99 - 113|
|Published online||08 March 2006|
Ph. Stee (ed)
EAS Publications Series, 18 (2006) 99-113
3D Continuum Radiative Transfer. An adaptive grid construction algorithm based on the Monte Carlo method
Observatorio Astronómico Nacional (IGN), Observatorio Astronómico de Madrid, Alfonso XII, 3, 28014 Madrid, Spain
Solving the radiative transfer problem is a common problematic to may fields in astrophysics. With the increasing angular resolution of spatial or ground-based telescopes (VLTI, HST) but also with the next decade instruments (NGST, ALMA, ...), astrophysical objects reveal and will certainly reveal complex spatial structures. Consequently, it is necessary to develop numerical tools being able to solve the radiative transfer equation in three dimensions in order to model and interpret these observations. I present a 3D radiative transfer program, using a new method for the construction of an adaptive spatial grid, based on the Monte Claro method. With the help of this tools, one can solve the continuum radiative transfer problem (e.g. a dusty medium), computes the temperature structure of the considered medium and obtain the flux of the object (SED and images).
© EAS, EDP Sciences, 2006
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