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Solar Flares with SMM and Implications for the Physics of Stellar Flares

Published online by Cambridge University Press:  12 April 2016

R. Pallavicini
R. Pallavicini*
Affiliation:
Arcetri Astrophysical Observatory, Florence, Italy

Abstract

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XUV flare observations from SMM are discussed and a comparison is made with recent X-ray observations of stellar flares.

Information

Type
Session III: Observed Activity in Related Objects
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 321 - 324
Copyright
Copyright © Reidel 1983

References

REFERENCES

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Pallavicini, R., Peres, G., Serio, S., Vaiana, G., Acton, L., Leibacher, J. : 1982, submitted to the Astrophys. J.Google Scholar