Author:
Daigne G.,Lantos-Jarry M. F.,Pick M.
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.
Publisher
Cambridge University Press (CUP)
Cited by
7 articles.
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