Bibcode
Bendicho, P. Fabiani
Referencia bibliográfica
Astrophysics and Space Science, v. 263, Issue 1/4, p. 223-226 (1998).
Fecha de publicación:
6
1998
Revista
Número de citas
0
Número de citas referidas
0
Descripción
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.