The relationship between the geomagnetic activity of the three years preceding a sunspot minimum and the peak of the next sunspot maximum confirms the polar origin of the solar wind during one part of the solar cycle. Pointing out that the polar holes have a very small size or disappear at the time
Solar cycle dependence of polar coronal holes
β Scribed by T. K. Das; T. N. Chatterjee; A. K. Sen
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 185 KB
- Volume
- 148
- Category
- Article
- ISSN
- 0038-0938
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