The evolution of the photospheric magnetic field pattern over eleven solar rotations preceding a minimum of the activity cycle is shown to be characterized by abrupt changes of the dominant geometrical patterns of the field. These changes are associated with the onset and end of a sudden increase in
Photospheric Magnetic Field of the Sun: Two Patterns of
โ Scribed by E. S. Vernova; M. I. Tyasto; D. G. Baranov
- Book ID
- 106532582
- Publisher
- Springer
- Year
- 2007
- Tongue
- English
- Weight
- 576 KB
- Volume
- 245
- Category
- Article
- ISSN
- 0038-0938
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