We study series of homologous flares, observed in the active region NOAA 2372 by the HXIS on the Solar Maximum Mission and ground based observatories. Changes in the flare homology, particularly those related to the location of the hard X-ray emission, show clear correlation with the development of
Two distinct morphological types of magnetic shear development and their relation to flares
β Scribed by H. Kurokawa
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 424 KB
- Volume
- 113
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
From a morphological study of the evolution of six active regions, we found two types of processes for the development of magnetic shear configurations between sunspots: (A) collision of two sunspots of opposite magnetic polarities, and (B) successive emergence of twisted magnetic flux ropes. We conclude that the process (B) might be essential for the production of major flares.
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