This paper discusses solar cosmic ray phenomena and related topics from the solar physical point of view. Basic physics of the solar atmosphere and solar flare phenomena are, therefore, considered in some detail. Since solar cosmic rays are usually produced by solar flares, we must first understand
Abstracts of papers from other journals
- Book ID
- 104646147
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 353 KB
- Volume
- 32
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
The paper presents an analysis of the longitudinal distribution of Ca u flocculi in the equatorial zone of ::k 20 heliographic degrees. Using the method of photographic surface integration, the regularity of the distribution of the flocctdi is investigated, considering various extents of statistical centring. On smoothing the material considerably, two longitudinal regions of preferred occurrence of Ca It floccuii, 180 ~ apart with a recurrence of 27.2 days, became outstanding. Comparisons were made of the papers of Bumba and Howard (1969), Dodson and Hedeman (1968), Svestka (1968), S3~kora (1971) and Vitinskij (1969), and the proportional effect of various methods of treatment on the results obtained was found. A periodic change in the distribution of the Ca II flocculae structure on the whole Sun was found with a mean period of 1.7 yr.
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