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The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI)
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) performs imaging spectroscopy of the Sun with high spatial and spectral resolution from 3 keV to 17 MeV using indirect Fourier-transform techniques. We review the rationale behind the RHESSI data analysis software, and explain the underlying structure of the software tools. Our goal was to make the large data set available within weeks after the RHESSI launch, and to make it possible for any member of the scientific community todoi:10.1007/978-94-017-3452-3_9 fatcat:gsafytpakva7dhnqotq25ht2zy