We determine the energy in the thermal and non-thermal parts of the RHESSI spectrum for a large selection of flares. The various flare parameters such as spectral index, source size and temperature are measured and analyzed statistically. TRACE observations are used if available to determine the energy of bulk motion. For details see paper by Saint-Hilaire and Benz in Solar Phys. 2002 (RHESSI First Results).
Participants: Pascal Saint-Hilaire and Arnold O. Benz