Non-Fourier description of heat flux evolution in 3D MHD simulations of the solar corona
Author:
Affiliation:
1. Max Planck Institute for Solar System Research, Göttingen, Germany
2. Gesellschaft für wissenschaftliche Datenverarbeitung mbH Göttingen, Göttingen, Germany
Publisher
Informa UK Limited
Subject
Geochemistry and Petrology,Mechanics of Materials,Geophysics,Astronomy and Astrophysics,Computational Mechanics
Link
https://www.tandfonline.com/doi/pdf/10.1080/03091929.2019.1670173
Reference52 articles.
1. The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun
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3. Nanoflare statistics in an active region 3D MHD coronal model
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5. Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region
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