Sunspot drawings obtained at National Astronomical Observatory of Japan during the years 1954-1986 were used to determine the differential rotation of the Sun. From the limited data set of three solar cycles it was found that three factors (the level of cycle activity, the cycle phase, and sunspot t
Solar rotation rate from stable sunspot tracings
✍ Scribed by Atila Özgüç; Mualla Sağlamsaatçi
- Publisher
- Springer Netherlands
- Year
- 1989
- Tongue
- English
- Weight
- 230 KB
- Volume
- 153
- Category
- Article
- ISSN
- 0004-640X
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