Magnetic field diagnostics of prominences with the Mg II k line 3D Stokes inversions versus traditional methods
The Mg II k resonance line is commonly used for diagnosing the solar chromosphere. We theoretically investigated its intensity and polarization in solar prominences, taking 3D radiative transfer and Hanle and Zeeman effects into account. We used an optically thick 3D model representative of a solar prominence and applied several inversion methods
Štěpán, Jiří et al.
Fecha de publicación:
9
2024