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Electron acceleration in solar flares: observations versus numerical simulations

Published online by Cambridge University Press:  01 August 2006

Arnold O. Benz ,
Paolo C. Grigis  and
Marco Battaglia
Arnold O. Benz
Affiliation:
Institute of Astronomy, ETH Zurich, 8092-Zurich, Switzerland email: [email protected]
Paolo C. Grigis
Affiliation:
Institute of Astronomy, ETH Zurich, 8092-Zurich, Switzerland email: [email protected]
Marco Battaglia
Affiliation:
Institute of Astronomy, ETH Zurich, 8092-Zurich, Switzerland email: [email protected]
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Abstract

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We use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally considered to be a primary recipient of the released energy.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 87
Copyright
Copyright © International Astronomical Union 2007

References

Battaglia, M., & Benz, A.O. 2007, A&A, 466, 713Google Scholar
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Grigis, P.C., & Benz, A.O. 2004, A&A 426, 1093Google Scholar
Grigis, P.C., & Benz, A.O. 2006, A&A, 458, 641Google Scholar
Lin, R.P., Dennis, B.R., Hurford, G.J., et al. 2002, Solar Phys., 210, 3CrossRefGoogle Scholar