9th RHESSI Workshop |
Genova, Italy, September 1-5 2009 |
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Alexander Warmuth Astrophysical Institute Potsdam, Germany Email: awarmuth (at) aip.de Group 2 Contribution: RHESSI spectroscopy is used combined with imaging to derive key parameters of both the thermal and nonthermal electron populations for a sample of solar flares ranging from C to X class. Implications for energy partition will be discussed. Group 4 Contribution: -
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