We have made number counts of the bright points that populate the interior of the Ca II network in the solar chromosphere for four solar cycles. We find that the number of these fine structures during the solar maximum exceeds that during the minimum phase on an average by 30%. The contribution due
โฆ LIBER โฆ
Global solar magnetology and reference points of the solar cycle
โ Scribed by V. N. Obridko; B. D. Shelting
- Book ID
- 110137053
- Publisher
- Springer
- Year
- 2003
- Tongue
- English
- Weight
- 396 KB
- Volume
- 47
- Category
- Article
- ISSN
- 1063-7729
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