A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum

DOI10.1051/0004-6361:20078834zbMath1140.85315OpenAlexW2126014346WikidataQ68672755 ScholiaQ68672755MaRDI QIDQ3502359

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Publication date: 23 May 2008

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1051/0004-6361:20078834

zbMATH Keywords

Sun: corona - Sun: magnetic fields - magnetohydrodynamics (MHD)

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (2)

Three-dimensional solutions of the magnetohydrostatic equations for rigidly rotating magnetospheres in cylindrical coordinates ⋮ Three-dimensional analytical magnetohydrostatic equilibria of rigidly rotating magnetospheres in cylindrical geometry

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