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X-ray,Hα, and radio observations of the two-ribbon flare of 16 May, 1981 |
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| Authors: | F Fárník J Kaastra B Kálmán M Karlický C Slottje B Valni?ek |
| Institution: | 1. Astronomical Institute of the Czechoslovak Academy of Sciences, 25165, Ond?ejov, Czechoslovakia 2. Astronomical Institute of the Rijksuniversiteit Utrecht, Zonnenburg 2, 3512, Utrecht, NL, Netherlands 3. Heliophysical Observatory of the Hungarian Academy of Sciences, H-4010, Debrecen, Hungary 4. Dwingeloo Observatory, N.F.R.A., P.O. Box 2, Dwingeloo, Netherlands |
| Abstract: | The paper is a contribution to the study of two-ribbon flares. A variety of observational material, i.e. Hα pictures, radio spectrum in the frequency band of 150–1000 MHz, radio map at 6 cm, fluxes at other frequencies, magnetograms and X-ray flux in a broad energy interval, enabled us to study the development of the 16 May, 1981 flare. The onset of the flare could be described by the model of Van Tend and Kuperus. A diminishing of the magnetic shear during the activation of the filament was observed. From radio and X-ray data it was found that pulsed acceleration took place in the region under the rising filament, the electrons propagating in a limited region both upwards to greater heights and downwards into the footpoints. Internal oscillations of the filament were observed. A manifestation of the primary process of interplanetary shock-wave generation was found. The 6 cm radio sources could be localized in the footpoints of magnetic loops. |
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