On the Determination of Magnetic Field Strength and Flux in Inter-Network
The results of the determination of magnetic field strength and flux from weak polarimetric signals in solar inter-network regions are contradictory. We investigate the origin of this contradiction with the help of MHD simulations. It is shown that the Stokes-V line ratio of the Fe I 5247/5250 Å and 15652/15648 Å line pairs is a good indicator of
Khomenko, E. et al.
Fecha de publicación:
12
2006