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Influence of magnetic fields on the structure of the solar corona∗
Published online by Cambridge University Press: 14 August 2015
Abstract
A current-free approximation to the coronal magnetic field is calculated from measured photospheric magnetic fields (Mt. Wilson) and traced by computer. The calculated field structure is then compared to a white-light photograph of the November 12, 1966 eclipse.
- Type
- Part V: Coronal and Interplanetary Structure of an Active Region
- Information
- Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 379 - 384
- Copyright
- Copyright © Reidel 1968
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