Some Statistical Properties of the Magnetic Field in Prominences
Abstract
Magnetic field observations based on the Zeeman effect, measuring the longitudinal component B∥ of the field with an entrance hole of 6.4 arcsec diameter, were obtained for a great number of prominences during 1979 to 1985.
- Publication:
-
The Role of Fine-Scale Magnetic Fields on the Structure of the Solar Atmosphere
- Pub Date:
- 1987
- Bibcode:
- 1987rfsm.conf..289K