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Electron acceleration in solar flares: observations versus numerical simulations
Published online by Cambridge University Press: 01 August 2006
Abstract
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