According to one of the most popular classifications, solar flares may be assigned either to the category of small short-lived events, or to the category of large, long-duration two-ribbon (2-R) flares. Even if such a broad division oversimplifies the flare phenomenon, our knowledge of the character
Cosmic-ray modulation and long-duration solar flare events
✍ Scribed by K. Kudela; A. Antalová; D. Venkatesan; J. Rybák
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 343 KB
- Volume
- 154
- Category
- Article
- ISSN
- 0038-0938
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