Radiative Transfer Under Inhomogeneous Configurations

Details Radiative Transfer Under Inhomogeneous Configurations Radiative Transfer Under Inhomogeneous Configurations

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..223b&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 223-226 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present, for the first time, three dimensional (3D) radiative transfer (RT) results with realistic atomic models (multilevel) and without using the local thermodinamical equilibrium approximation (non-LTE). We have developed a new code based on efficient iterative methods (Trujillo Bueno, and Fabiani Bendicho 1995; Fabiani Bendicho, Trujillo Bueno and Auer 1997) characterized by a very high convergence rate. With this 3D multilevel code and using a schematic atmospheric model we are able to demonstrate that one may need self-consistent multidimensional RT calculations in order to interpret high spatial resolution solar spectroscopic observations.

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