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The Solar Corona over the Recent Saros

Published online by Cambridge University Press:  12 April 2016

Jay M. Pasachoff
Jay M. Pasachoff*
Affiliation:
Williams College-Hopkins Observatory, Williamstown, Mass. 01267, USA; Institute for Advanced Study, Princeton, N.J. 08540, USA

Abstract

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We are now at both the maximum of the solar activity cycle and at the most populated part of the saros. I discuss the solar corona over the recent saros and its changes with the solar activity cycle. We consider the scientific value of eclipse studies and how they relate to other ongoing coronal studies on the sun and other stars.

Type
Part III Solar magnetism and large-scale flows
Information
International Astronomical Union Colloquium , Volume 130: The Sun and Cool Stars: activity, magnetism, dynamos , 1991 , pp. 285 - 287
Copyright
Copyright © Springer-Verlag 1991

References

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