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A.G. Emslie (Department of Physics, UAH)
We present preliminary results on the spatial distribution of solar flare hard X-ray emission as observed by the RHESSI spacecraft. Particular attention will be paid to the variation of the hard X-ray, and hence electron, flux spectra throughout the source structure and their attendant implications for models of electron acceleration and transport in solar flares.
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.