Formation of neutral current sheet and loop coronal transients

Details Formation of neutral current sheet and loop coronal transients Formation of neutral current sheet and loop coronal transients

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987chjss...7....1h&link_type=abstract

(Chinese Journal of Space Science, vol. 7, no. 1, 1987, p. 1-9) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 11, Ju

Statistics

Computation

Coronal Loops, Current Sheets, Magnetic Flux, Neutral Currents, Solar Corona, Solar Magnetic Field, Computational Astrophysics, Magnetoacoustic Waves, Solar Atmosphere, Solar Flares

Scientific paper

Starting from the equations for an ideal magnetic fluid, a numerical investigation of the formation of a neutral current sheet from the eruption of opposite magnetic flux and the accompanying responses in the coronal atmosphere is performed, taking into account the interaction between the magnetic field and the coronal plasma. The results show the typical prominence/tenuous region/dense loop/forerunner region structure shown by coronal loop transients. These findings confirm the previous suggestion that injection of opposite magnetic flux into a dipole background is probably an important mechanism in the formation of loop coronal transients.

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