An active region filament studied simultaneously in the chromosphere and photosphere

2011/12/07 by C. Kuckein, V. Martínez Pillet, V. Martinez Pillet +1 · 1 citation
Physics and Astronomy · #Chromosphere #Field (mathematics) #Ionosphere and magnetosphere dynamics #Magnetic field #Photosphere #Protein filament #Scientific Research and Discoveries #Solar and Space Plasma Dynamics #Solar prominence #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201117675

Accepted for publication in Astronomy & Astrophysics, 16 pages, 13 figures

arxiv created 2011/12/07 · openalex publication_date 2012/01/09 · arxiv updated 2015/06/03 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. A thorough multiwavelength, multiheight study of the vector magnetic field in a compact active region filament (NOAA 10781) on 2005 July 3 and 5 is presented. We suggest an evolutionary scenario for this filament.

Citations

• Signatures of Incomplete Paschen‐Back Splitting in the Polarization Profiles of the Heiλ10830 Multiplet
• Twisted Flux Tube Emergence From the Convection Zone to the Corona
• PROMINENCE FORMATION ASSOCIATED WITH AN EMERGING HELICAL FLUX ROPE

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