Flare build-up in preflare low-lying loops and nonlinear force-free magnetic field

Details Flare build-up in preflare low-lying loops and nonlinear force-free magnetic field Flare build-up in preflare low-lying loops and nonlinear force-free magnetic field

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21..152s&link_type=abstract

Acta Astronomica Sinica, vol. 21, June 1980, p. 152-157. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

2

Coronal Loops, Force-Free Magnetic Fields, Nonlinear Equations, Solar Flares, Solar Magnetic Field, Electric Current, Magnetic Field Configurations, Solar Protons, Temperature Dependence

Scientific paper

Low's study of nonlinear force-free magnetic fields (1977) is used to explain the preflare low-lying magnetic loop phenomenon observed by Skylab. It is shown that higher magnetic loops evolve toward low-lying loops when the shear angle between the magnetic field line and the magnetic neutral line increases with time and the foot points of the magnetic field line move close to the neutral line. It is suggested that low-lying loops are responsible for the buildup of proton flares.

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