An interesting aspect of solar rotation is the fact that coronal holes seem to exhibit little or no differential rotation. We set out to investigate the question of whether or not the photospheric magnetic fields underlying coronal holes also exhibit reduced differential rotation. In order to accomp
β¦ LIBER β¦
Reorientation of global coronal magnetic fields due to differential rotation
β Scribed by Shirley F. Hansen; Richard T. Hansen
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 423 KB
- Volume
- 51
- Category
- Article
- ISSN
- 0038-0938
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