3-D MHD simulation of the generation of a shell current loop with closure current

Details 3-D MHD simulation of the generation of a shell current loop with closure current 3-D MHD simulation of the generation of a shell current loop with closure current

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..156..281s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 156, no. 2, p. 281-292

Physics

3

Loops, Magnetohydrodynamics, Plasma Currents, Plasmas (Physics), Shells (Structural Forms), Simulation, Coronal Loops, Magnetic Fields, Plasma Density, Solar Flares, Solar Physics, Sun

Scientific paper

We present results for the generation process of a shell current loop by using a three-dimensional ideal MHD code. It is shown that a shell current loop with a diffuse closure current can be generated due to the twisting motions of the loop footpoints. It is also shown that during the generation of a shell current loop, plasma density enhancement propagates along a shell current loop. It is suggested that the generation process of a shell current loop may be related to the movement of soft X-ray enhancement from the footpoints along a loop before onset of a solar flare.

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