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Correlations between brightness fields and magnetic fields on the Sun∗
Published online by Cambridge University Press: 14 August 2015
Abstract
In places on the solar surface where longitudinal magnetic fields are detectable using Leighton's photographic technique, spectroheliograms taken in the cores of many Fraunhofer lines show a bright photospheric network similar to, but with finer structure than, the familiar chromospheric network visible on Ca+ K232 spectroheliograms. This paper describes preliminary results of a study of the relation between the photospheric network and its associated magnetic fields.
- Type
- Part III: Optical Structure of an Active Region
- Information
- Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 161 - 173
- Copyright
- Copyright © Reidel 1968