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Inversion Lines of Photospheric Magnetic Fields and Solar Corona

Published online by Cambridge University Press:  25 May 2016

F. Axisa ,
M.-J. Martres  and
C. Mercier
F. Axisa
Affiliation:
Service d'Electronique Physique, Centre d'études Nucléaires de Saclay, France
M.-J. Martres
Affiliation:
Solar Dept. Meudon Observatory, 92190 Meudon, France
C. Mercier
Affiliation:
Solar Dept. Meudon Observatory, 92190 Meudon, France

Abstract

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(Solar Phys.). Two results were obtained recently at Meudon concerning the metric type III production by flares which both emphasize the importance of the local magnetic configuration involved.

Type
Part I Magnetic Structure Responsible for Coronal Disturbances
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 69 - 72
Copyright
Copyright © Reidel 1974 

References

Axisa, F.: 1974, Solar Phys. 35, 207–224.Google Scholar
Mercier, C.: 1973, Solar Phys. 33, 177.Google Scholar