The N-S drift of sunspot groups has been studied in a different way than previously, using positions of recurrent groups of the years 1874-1976. The existence of the meridional motions, the general shape of the drift curves, and the dissimilarity between these curves around sunspot maxima and minima
Temporal Variations of the Solar Rotation Determined by Sunspot Groups
✍ Scribed by R. Brajša; D. Ruždjak; H. Wöhl
- Publisher
- Springer
- Year
- 2006
- Tongue
- English
- Weight
- 339 KB
- Volume
- 237
- Category
- Article
- ISSN
- 0038-0938
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