Signatures of Incomplete Paschen-Back Splitting in the Polarization Profiles of the He I λ10830 Multiplet
Abstract
We investigate the formation of polarization profiles induced by a magnetic field in the He I multiplet at 10830 Å. Our analysis considers the Zeeman splitting in the incomplete Paschen-Back regime. The effects turn out to be important and produce measurable signatures on the profiles, even for fields significantly weaker than the level-crossing field (~400 G). When compared to profiles calculated with the usual linear Zeeman effect, the incomplete Paschen-Back profiles exhibit the following conspicuous differences: (1) a non-Doppler blueshift of the Stokes V zero-crossing wavelength of the blue component; (2) area and peak asymmetries, even in the absence of velocity and magnetic gradients; and (3) a ~25% reduction in the amplitude of the red component. These features do not vanish in the weak-field limit. The spectral signatures that we analyze in this paper may be found in previous observations published in the literature.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 2004
- DOI:
- 10.1086/422580
- arXiv:
- arXiv:astro-ph/0409005
- Bibcode:
- 2004ApJ...612.1175S
- Keywords:
-
- Line: Profiles;
- Sun: Atmosphere;
- Sun: Chromosphere;
- Sun: Magnetic Fields;
- Astrophysics
- E-Print:
- Accepted for publication in The Astrophysical Journal