Physics – Plasma Physics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..219s&link_type=abstract
In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 219-221 (SEE N94-22624 05-75)
Physics
Plasma Physics
1
Coronal Loops, Magnetic Field Configurations, Magnetohydrodynamics, Plasma Dynamics, Solar Corona, Solar Flares, Taylor Instability, Two Dimensional Flow
Scientific paper
In order to reveal the solar flare mechanism, the dynamics, as well as the equilibria, in solar coronal magnetic loops and arcade are investigated using the numerical simulations. The main objectives are the following: to achieve the solution of Taylor's minimum energy state for the magnetic arcade; to investigate the two dimensional dynamics in a magnetic arcade by numerical simulations; and to investigate the three dimensional dynamics in magnetic loops by numerical simulations. A loop-loop interaction is observed when the magnetic energy and helicity are injected by a rotating motion on foot points of loops.
Kubo Hiroko
Kusano Kanya
Nishikawa Kyoji
Sato Tetsuya
Suzuki Yoshio
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