The dynamical process of a coronal transient associated with an eruptive prominence. I. Basic mechanism

DOI10.1007/BF00651302zbMath0523.76097OpenAlexW3094010873MaRDI QIDQ1056643

Wen-rui Hu

Publication date: 1983

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00651302

zbMATH Keywords

method of characteristicspiston modelactive phenomenabase regioncoronal transienteruptive prominences and flaresrarefaction region in lower coronasolartop region

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (2)

The dynamical process of a coronal transient associated with an eruptive prominence. II. Analytical solutions in finite regions ⋮ One-dimensional piston process in strong gravitational field

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