Article contents
Magnetic Field and Turbulence in Sunspots
Published online by Cambridge University Press: 14 August 2015
Abstract
We study the local variations of η0 and ξ (Milne-Eddington model) which are necessary in order to bring in agreement three independent determinations of the total field H, obtained from simultaneous observations of the two lines λ 5250,2 Fe I and λ 5225,5 Fe I. The distribution of the broadening as a function of field direction is consistent with the motions induced by hydromagnetic waves.
- Type
- Part III: Observations of Sunspot and Active Region Magnetic Fields
- Information
- Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 181 - 189
- Copyright
- Copyright © Reidel 1971
References
- 2
- Cited by