Re-interpretation of OSO-III scintillation counter measurements of hard solar X-ray spectra |
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| Authors: | S. R. Kane H. S. Hudson |
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| Affiliation: | (1) Space Sciences Laboratory, University of California, 94720 Berkeley, Calif., U.S.A.;(2) Dept. of Physics, University of California, 92038 San Diego, La Jolla, Calif., U.S.A. |
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| 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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