Micro-structured magnetic atmospheres
Asymmetrical Stokes profiles are produced if the photospheric magnetic and velocity fields are structured on scales smaller than the mean-free-path of the photons. Here we put forward a compact analytical expression for the radiative transfer equation in this case. Explicitly, micro-variations of the magnetic field strength and the velocity are
Sánchez Almeida, J. et al.
Fecha de publicación:
3
1996