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Magnetic Structure Responsible for Coronal Disturbances: Observations

Published online by Cambridge University Press:  25 May 2016

Martin D. Altschuler
Martin D. Altschuler*
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research*, Boulder, Colo., U.S.A.

Abstract

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Coronal disturbances are considered as consequences of the ejection of electric currents (or non-potential magnetic fields) from the photosphere and chromosphere into the corona. It may be that electric currents are generated near neutral lines in the photosphere and are later ejected into the corona.

Type
Part I Magnetic Structure Responsible for Coronal Disturbances
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 3 - 33
Copyright
Copyright © Reidel 1974 

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