Abstract
Laboratory tests show that pulse pile-up requires a significant correction to the response of scintillation counters to solar X-ray bursts with steep energy spectra. The interpretation of the OSO-III and other satellite data in view of these corrections indicates that steep solar X-ray spectra with varying emission measure produce an effect similar to that produced by relatively hard spectra with a constant emission measure.
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Kane, S.R., Hudson, H.S. Re-interpretation of OSO-III scintillation counter measurements of hard solar X-ray spectra. Sol Phys 14, 414–418 (1970). https://doi.org/10.1007/BF00221327
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DOI: https://doi.org/10.1007/BF00221327