Computer Science – Numerical Analysis
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115...93a&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 115, no. 1, 1988, p. 93-106.
Computer Science
Numerical Analysis
5
Magnetic Field Configurations, Magnetohydrodynamics, Mass Transfer, Solar Magnetic Field, Solar Prominences, Chromosphere, Condensing, Conductive Heat Transfer, Gravitational Effects, Numerical Analysis, Plasma Density
Scientific paper
A two-dimensional MHD model simulating the formation of Kippenhahn-Schluter (1957) quiescent prominence (QP) magnetic field configurations is used to explore symmetric mass injection into a dipole magnetic field. An optimum magnetic field strength for QP formation by mass injection is obtained. It is found that a weaker magnetic field strength is more favorable for the condensation of the injected plasma but that a stronger field is more favorable for supporting the condensed plasma against gravity.
An Chang-Hyuk
Bao Jingdong
Suess Steve T.
Wu Shi Tsan
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