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- W2040372384 abstract "A balloon-borne measurement of the cosmic ray electron spectrum from 10 to 200 Gev is reported in which two new techniques have been used to remove proton background contamination. First, the depth of the spectrometer was more than 40 radiation lengths, the equivalent of more than 3 mean free paths of material, enabling hadronically and electromagnetically induced cascades to be differentiated for a subset of the data. Second, electromagnetic cascade starting points were determined to within ±0.1 radiation lengths on the basis of a calibration with electrons from 5.4 to 18 Gev at the Stanford Linear Accelerator, greatly reducing the chances for a proton to simulate an electron. The resulting spectrum, when fitted with a power law, is quite steep, −3.2 ± 0.1, but the fit to a power law is marginal." @default.
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- W2040372384 date "1973-11-01" @default.
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- W2040372384 title "Primary cosmic ray electrons above 10 Gev: Measurements using a thick detector" @default.
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- W2040372384 doi "https://doi.org/10.1029/ja078i031p07165" @default.
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