Milne-Eddington inversions of the He I10 830 Å Stokes profiles: influence of the Paschen-Back effect

2006/08/04 by C. Sasso, A. Lagg, S. K. Solanki · 3 citations
Physics and Astronomy · #Atmospheric models #Helioseismology #Magnetic confinement fusion research #Multiplet #Position (finance) #Quantum, superfluid, helium dynamics #Solar and Space Plasma Dynamics #Zeeman effect #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361:20065257

published as A&A 456, 367-371 (2006) · Accepted for publication in A&A on Jun 12th 2006

openalex publication_date 2006/08/04 · arxiv created 2011/02/04 · arxiv updated 2015/03/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context.The Paschen-Back effect influences the Zeeman sublevels of the multiplet at 10 830 Å, leading to changes in strength and in position of the Zeeman components of these lines.

Citations

• Signatures of Incomplete Paschen‐Back Splitting in the Polarization Profiles of the Heiλ10830 Multiplet

Cited by

• Inversion of the radiative transfer equation for polarized light
• Three-dimensional magnetic structure of a sunspot: Comparison of the photosphere and upper chromosphere
• An active region filament studied simultaneously in the chromosphere and photosphere