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The Scaling of Solar Flare Hard X-ray Emission to Other Flaring Objects in the Universe

Published online by Cambridge University Press:  25 May 2016

P. C. H. Martens
P. C. H. Martens*
Affiliation:
Department of Physics, Montana State University—Bozeman, Bozeman, MT 59717-3840, U.S.A.

Abstract

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Fletcher & Martens have successfully modeled solar hard X-ray sources observed at the top and footpoints of flaring magnetic loops with a Fokker-Planck type particle transport code. I show here that there are invariances in the Fokker-Planck equations that make these results applicable to environments with vastly different physical parameters, such as hard X-ray flares in accretion disks in active galactic nuclei, and in RS CVn and ALGOL type binaries.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 133 - 134
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

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