Zeeman line formation in solar magnetic fields

Author:

Sampoorna M.,Nagendra K. N.,Frisch H.,Stenflo J. O.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference37 articles.

1. Meso-structured magnetic atmospheres: Stochastic polarized radiative transfer and Stokes profile inversion

2. Line formation in turbulent magnetic atmospheres

3. Carroll, T. A., & Staude, J. 2005b, ESA SP-596: Chromospheric and Coronal Magnetic Fields, ed. D. E. Innes, A. Lagg, & S. K. Solanki, 30 August 2005, Katlenburg-Lindau, Germany, published on CDROM, 9.1

4. Carroll, T. A., & Staude, J. 2006, Solar Polarization 4, ed. R. Casini, & B. W. Lites, 19 September 2005, National Center for Atmospheric Research, Boulder, Colorado, USA, ASP Conf. Ser., 358, 137

5. The meso-structured magnetic atmosphere

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