We have measured the longitudinal component, Bll, of the magnetic field in quiescent prominences and obtained a relationship between BII and 0, where 0 is the angle between the long axis of the prominence and the north-s0uth direction on the sun. From this relationship we deduce a distribution funct
โฆ LIBER โฆ
Parameters of quiescent prominences derived from magnetic field measurements
โ Scribed by Ulrich Anzer
- Publisher
- Springer
- Year
- 1995
- Tongue
- English
- Weight
- 379 KB
- Volume
- 161
- Category
- Article
- ISSN
- 0038-0938
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