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Expulsion of Magnetized Plasmas from Coronae

Published online by Cambridge University Press:  04 August 2017

B. C. Low
B. C. Low*
Affiliation:
High Altitude Observatory National Center for Atmospheric Research1 Boulder, Colorado, USA

Abstract

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A theory of the white light transient phenomena in the solar corona is given, based on recent analytic treatments of magnetohydrodynamics.

Type
V. Stellar Winds and Spindown in Late — Type Stars
Information
Symposium - International Astronomical Union , Volume 102: Solar and Stellar Magnetic Fields: Origins and Coronal Effects , 1983 , pp. 467 - 471
Copyright
Copyright © Reidel 1983 

References

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