The Feb 4 1986 flare and filament current loop coalescence instability.

Details The Feb 4 1986 flare and filament current loop coalescence instability. The Feb 4 1986 flare and filament current loop coalescence instability.

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acasn..36..301t&link_type=abstract

Acta Astron. Sin., Vol. 36, No. 3, p. 301 - 308

Astronomy and Astrophysics

Astronomy

Solar Flares: Observations, Solar Filaments: Loops, Solar Filaments: Instabilities

Scientific paper

The observational data of Hα, radio, soft X-ray, hard X-ray and γ-ray for the 3B/3X flare on Feb 4, 1986 are collected. This flare is studied comprehensively by using the flare-filament current model. The results show that (1) the 3B/X3 flare on Feb 4, 1986 was possibly caused by the current loop coalescence instability between two filament current loops; (2) the resistive tearing instability is an efficient pre-heating mechanism of pre-flare phase; (3) the high energy data on the Feb 4 flare further corroborate that the current loop coalescence instability is a possibly efficient mechanism for the simultaneous acceleration of high energy particles during the flare.

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