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Optical and Radio Observations of Large Scale Magnetic Fields on the Sun
Published online by Cambridge University Press: 14 August 2015
Abstract
It is possible to deduce information concerning large scale coronal magnetic field patterns from the knowledge of the location of radioburst sources.
As the method concerns active centers responsible for corpuscular emission, the knowledge of these structures may have important implications in the understanding of corpuscular propagation in the corona and in the interplanetary medium.
- Type
- Part VI: Optical and Radio Observations of Large Scale Magnetic Fields on the Sun
- Information
- Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 609 - 615
- Copyright
- Copyright © Reidel 1971
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