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Link between the chromospheric network and magnetic structures of the corona

2006/09/11 by Stefan Jendersie, Hardi Peter · 1 citation
Physics and Astronomy · #Astrobiology #Astrophysics #Context (archaeology) #Corona (planetary geology) #Coronal mass ejection #Extrapolation #Geology #Ionosphere and magnetosphere dynamics #Magnetic field #Magnetic flux #Nanoflares #Photosphere #Physics #Solar and Space Plasma Dynamics #Solar wind #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066166

8 pages, 5 figures, acceped for publication in A&A

arxiv created 2006/09/11 · openalex publication_date 2006/09/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. Recent work suggested that the traditional picture of the corona above the quiet Sun being rooted in the magnetic concentrations of the chromospheric network alone is strongly questionable.

Citations

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