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The flares of April 1980 |
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| Authors: | Marcos E Machado Boris V Somov Marta G Rovira Cornelis De Jager |
| Institution: | 1. Observatorio de Física Cósmica - CNIE, 1663, San Miguel, Argentina 2. P.N. Lebedev Physical Institute, Moscow, U.S.S.R. 3. I.A.F.E., Buenos Aires, Argentina 4. Space Research Laboratory, Utrecht, The Netherlands |
| Abstract: | We discuss the spatial and temporal characteristics of X-ray flares occurring in the active region NOAA2372 from April 6 to 13, 1980. The flares are seen to extend in most cases across the whole active complex, involving several magnetic features. They originate in an intermediate bipole, between the two main sunspots of the active region, where high magnetic shear was detected. A rapid expansion is seen in some cases, in conjunction with the start of the impulsive hard X-ray bursts. We also detect, in the late phases of some of the events, a large soft X-ray structure overlying the whole active region, which also shows up as a noise storm region at metric wavelengths. These large loops cool by heat conduction but, in some cases, Hα condensations seem to appear, probably as a result of magnetic compression and a condensation mode of the thermal instability. The topological aspects of the field configuration are discussed, in the context of flare models invoking magnetic reconnection at the site of the primary energy release. In such a model, the intermediate bipole is the natural site of initial magnetic reconnection, particle acceleration and heating. In one particular case of a flare observed at the limb, we find possible evidence of particle acceleration in a neutral sheet at the boundary between two clearly defined magnetic structures. |
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