An Hermitian Method for the Solution of Polarized Radiative Transfer Problems
Spectral synthesis calculations in stellar (magnetized) atmospheres are based on the solution of the radiative transfer equation (RTE) for polarized light. The thermodynamic and magnetic properties of the atmospheres, along with the radiation field, completely specify the basic ingredients of the RTE, after which numerical methods have to be
Bellot Rubio, L. R. et al.
Fecha de publicación:
10
1998