Intermittent heating in the solar corona employing a 3D MHD model

DOI10.1051/0004-6361/201016019zbMath1260.85031arXiv1103.6042OpenAlexW3101213253WikidataQ68998816 ScholiaQ68998816MaRDI QIDQ4905727

Sven Bingert, Hans-Jörg Peter

Publication date: 20 February 2013

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

Full work available at URL: https://arxiv.org/abs/1103.6042

zbMATH Keywords

methods: numericalstars: coronaeSun: coronamegnetohydrodynamics (MHD)

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items (3)

The time step constraint in radiation hydrodynamics ⋮ Testing Alfvén wave propagation in a “realistic” set-up of the solar atmosphere ⋮ Non-Fourier description of heat flux evolution in 3D MHD simulations of the solar corona

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