Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasj...47..323i&link_type=abstract
PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 47, no. 3, p. 323-330
Astronomy and Astrophysics
Astronomy
22
Coronal Loops, Magnetic Field Reconnection, Magnetic Flux, Particle Acceleration, Solar Flares, X Ray Astronomy, X Ray Imagery, X Ray Spectra, High Energy Electrons, Image Analysis, Japanese Spacecraft, Morphology, Radiant Flux Density, Spectrum Analysis, Stellar Models, X Ray Telescopes
Scientific paper
Observations with the Soft X-ray and Hard X-ray Telescopes (SXT and HXT) aboard Yohkoh of simple solar flare on 1992 December 9 are discussed. The soft X-ray morphology suggests evidence of a loop-loop interaction mechanism: the images reveal two parallel magnetic loops prior to the flare, and their merging just before onset of the hard X-ray burst. This flare therefore provides a chance to examine the two-loop interaction model for solar flares. It is found (1) that the observed soft X-ray behavior of the two loops in the preflare phase well matches to the two-loop interaction model between strong and weak current loops and (2) that the observed time scale of the two-loop coalescence is almost equal to that estimated from explosive-reconnection theory. In the impulsive phase, it is found (3) that the loop-top portion near to the interaction region first brightens in the 14-23 keV hard X-rays and (4) that the 23-33 keV hard X-ray emission around the peak time originates dominantly from two compact sources at the two ends of the merging loops. These hard X-ray observations are explained by high-energy electrons that are produced in the two current loop interaction.
Inda-Koide Mika
Koide Shinji
Kosugi Takeo
Sakai Jun-Ichi
Sakao Taro
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