An active region filament studied simultaneously in the chromosphere and photosphere

2012/04/26 by C. Kuckein, V. Martínez Pillet, V. Martinez Pillet +1 · 45 citations
Earth and Planetary Sciences · Physics and Astronomy · #Atmospheric Ozone and Climate #Chromosphere #H-alpha #Ionosphere and magnetosphere dynamics #Photosphere #Protein filament #Solar and Space Plasma Dynamics #Solar atmosphere #Solar prominence #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201218887

published in Astronomy and Astrophysics 542, A112 (EDP Sciences) · Accepted for publication in Astronomy & Astrophysics, 15 pages, 8 figures, 4 tables; LaTeX links added, typos added, references updated

openalex publication_date 2012/04/26 · arxiv created 2014/01/13 · arxiv updated 2014/01/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Paper I presents the magnetic structure, inferred for the photosphere and the chromosphere, of a filament that developed in active region (AR) NOAA 10781, observed on 2005 July 3 and July 5.

Citations

• Signatures of Incomplete Paschen‐Back Splitting in the Polarization Profiles of the Heiλ10830 Multiplet
• Milne-Eddington inversions of the He I10 830 Å Stokes profiles: influence of the Paschen-Back effect
• Solar Surface Emerging Flux Regions: A Comparative Study of Radiative MHD Modeling andHinodeSOT Observations
• Frequent Occurrence of High‐Speed Local Mass Downflows on the Solar Surface
• Twisted Flux Tube Emergence From the Convection Zone to the Corona
• CORONAL RAIN AS A MARKER FOR CORONAL HEATING MECHANISMS
• PROMINENCE FORMATION ASSOCIATED WITH AN EMERGING HELICAL FLUX ROPE
• An active region filament studied simultaneously in the chromosphere and photosphere

Cited by

• Observational Evidence of a Flux Rope within a Sunspot Umbra