Physics
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..108..169w&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 108, no. 1, 1987, p. 169-181.
Physics
7
H Alpha Line, Solar Flares, Solar Radio Bursts, Solar X-Rays, Visual Observation, Electron Acceleration, Electron Energy, Flux Density, High Temperature Plasmas, Plasma Heating, Solar Maximum Mission
Scientific paper
The 2B/X2.8 double-ribbon flare of 30 March, 1982 is investigated using Hα, white light, X-rays and microwaves. The X-ray burst seems to consist of two components, i.e., an impulsive component showing a long chain of peaks and a thermal component (T ≡ 2×107K). A peak of one-directional intensity distribution at 35 GHz always lies on the core of the hard X-ray source, showing a shift of the position synchronous with the hard X-ray core. This may imply a common source for the radio waves and the hard X-rays. The source of the thermal component observed at the soft X-rays (7 - 14 keV) after the early phase covers a whole Hα patch. This may imply a physical relation between the thermal X-ray loops and the Hα brightening.
Kawabata Kiyoshi
Liu Qing-Jun
Ohki Kenichiro
Takakura Tastuo
Wang Jane-Ling
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