Observation of the impulse phase of a simple flare

Details Observation of the impulse phase of a simple flare Observation of the impulse phase of a simple flare

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90...41t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Jan. 1984, p. 41-62. NASA-supported research.

Physics

11

Solar Flares, Solar Magnetic Field, Solar Radio Bursts, Solar X-Rays, Magnetic Field Configurations, Plasma Acceleration, Plasma Heating, Solar Electrons, Solar Spectra, Spectroheliographs, Ultraviolet Spectra

Scientific paper

The paper presents a broad range of complementary observations (SMM and ground-based) of the onset and impulsive phase of the fairly large (1B, M1.2) but simple two-ribbon flare which occurred at 19:15 UT on November 1, 1980 in the northern part of the active region Boulder No. AR2776. It is found that the overall magnetic field configuration in which the flare occurred was a fairly simple, closed arch containing nonpotential substructure; the flare occurred spontaneously within the arch (it was not triggered by emerging magnetic flux). The two major spikes of the impulsive energy release are examined, and the three immediate products of this energy release are discussed.

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