Optical Tomography of a Sunspot. II. Vector Magnetic Field and Temperature Stratification
An observational determination of the three-dimensional magnetic and thermal structure of a sunspot is presented. It has been obtained through the application of the SIR inversion technique (Stokes Inversion based on Response functions) on a low-noise, full Stokes profile two-dimensional map of the sunspot as observed with the Advanced Stokes
Westendorp Plaza, C. et al.
Fecha de publicación:
2
2001