Flare build-up in low-lying magnetic loops

Details Flare build-up in low-lying magnetic loops Flare build-up in low-lying magnetic loops

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981cha%26a...5..123s&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 5, Issue 2, p. 123-127.

Astronomy and Astrophysics

Astrophysics

Scientific paper

B. C. Low's study on non-linear force-free magnetic field is extended in an effort to explain the preflare low-lying magnetic loops observed by Skylab. Using Low's method of analytical continuation, a revised boundary-value problem is solved analytically. It is shown that high magnetic loops will evolve into low-lying ones when both the shear angle between field line and the neutral line increases with time and the foot-points of the field lines close upon the neutral line. The density, temperature and electric current density are high in these lowlying loops, thus providing conditions for flare (especially proton flare) build-up.

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