Zeeman-tomography of the solar photosphere

2008/01/09 by T. A. Carroll, M. Kopf · 3 citations
Physics and Astronomy · #Solar and Space Plasma Dynamics #Spectroscopy and Quantum Chemical Studies #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079197

accepted for A&A Letters

openalex publication_date 2008/01/09 · arxiv created 2008/03/07 · arxiv updated 2009/12/01 · openalex created_date 2022/10/02 · openalex updated_date 2026/06/17

Abstract

Aims.The thermodynamic and magnetic field structure of the solar photosphere is analyzed by means of a novel 3-dimensional spectropolarimetric inversion and reconstruction technique.

Cited by

• A fast method for Stokes profile synthesis
• Magnetic field distribution in the quiet Sun: a simplified model approach
• Inversion of the radiative transfer equation for polarized light
• The magnetic flux of the quiet Sun internetwork as observed with the Tenerife infrared polarimeter

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