Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-19T04:44:43.128Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

de Vries, M., & Kuijpers, J. 1992, A&A, 266, 77.Google Scholar
Fletcher, L., & Martens, P. C. H. 1998, ApJ, 505, 418.Google Scholar
Masuda, S., Kosugi, T., Hara, H., Tsuneta, S., & Ogawara, Y. 1994, Nature, 371, 495.Google Scholar
van den Oord, G. H. J., Mewe, R., & Brinkman, A. C. 1988, A&A, 205, 181.Google Scholar