High resolution hard X-ray spectra of solar and cosmic sources
High resolution (('(TURN))1 keV) hard X-ray (14-300 keV) observations of a large solar flare and the Crab Nebula were obtained during balloon flights on October 18, 1979 and June 27, 1980 using an array of cooled germanium planar detectors. In addition, high time resolution (.128 sec.) high sensitivity measurements were obtained with a 300cm('2) NaI/CsI phoswich scintillator.
"High resolution (('(TURN))1 keV) hard X-ray (14-300 keV) observations of a large solar flare and the Crab Nebula were obtained during balloon flights on October 18, 1979 and June 27, 1980 using an array of cooled germanium planar detectors. In addition, high time resolution (.128 sec.) high sensitivity measurements were obtained with a 300cm('2) NaI/CsI phoswich scintillator."@en
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University of California, Berkeley. Department of Physics.
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