tokens: We are grateful to the referee for the constructive input which helped improve the paper. M.A. is grateful to Kim Tolbert and Richard Schwartz for useful discussions on uncertainty computation and general use of RHESSI data analysis tools. Thanks to Brian Dennis for his comments on making the best possible images with RHESSI and for numerous science discussions, and to Joel Allred for helpful discussions on the relative importance of energy loss mechanisms in solar plasmas. This work was supported by a NASA Heliophysics Guest Investigator grant and the RHESSI project.
ner_tags: O O O O O O O O O O O O O O O B-Person O O O B-Person I-Person O B-Person I-Person O O O O O O O O O O B-Telescope O O O O O B-Person I-Person O O O O O O O O O O B-Telescope O O O O O O O B-Person I-Person O O O O O O O O O O O O O O O O O O O O B-Organization B-Grant I-Grant I-Grant I-Grant O O B-Mission I-Mission