The magnetic polarity distributions in sunspot groups which produced solar proton flares have been analyzed. It is shown that the fluid motion in sunspot groups and below may be responsible for the origin of inverted or unusual polarity distributions, since rotating motion in these spot groups is of
✦ LIBER ✦
Sunspot motions and magnetic shears as precusors of flares
✍ Scribed by L. Dezső; G. Csepura; O. Gerlei; Á. Kovács; I. Nagy
- Publisher
- Elsevier Science
- Year
- 1984
- Tongue
- English
- Weight
- 249 KB
- Volume
- 4
- Category
- Article
- ISSN
- 0273-1177
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