1971
DOI: 10.1016/0370-2693(71)90130-4
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Absolute measurement of the vertical cosmic ray muon intensity at 3 – 50 GeV/c near sea level

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Cited by 36 publications
(20 citation statements)
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“…The comparison to low energy experiments [38][39][40][41][42][43] gives a good overall agreement with this analysis above about 40 GeV. At lower momenta, a systematic slope difference seems to be present, which corresponds to about three standard deviations of the systematic molasse uncertainty estimated above.…”
Section: Resultssupporting
confidence: 81%
See 1 more Smart Citation
“…The comparison to low energy experiments [38][39][40][41][42][43] gives a good overall agreement with this analysis above about 40 GeV. At lower momenta, a systematic slope difference seems to be present, which corresponds to about three standard deviations of the systematic molasse uncertainty estimated above.…”
Section: Resultssupporting
confidence: 81%
“…8. Only measurements providing an absolute normalization [36][37][38][39][40][41][42][43][44] are taken into account. The data are extrapolated to sea level using the muon flux predictions of the TARGET [20] program.…”
Section: Resultsmentioning
confidence: 99%
“…Table 1 lists the authors and energy range of the reported absolute vertical intensity measurements. It is also shown if the experiment has been used by other reviews, namely "B" (Bugaev et al, 1998), "H&T" (Hebbeker and Timmermans, 2002) Ayre et al (1975) 20-500 X X Baber et al (1968) 11-810 X X Rastin (1984) 3-3000 X 0.933 X Bateman et al (1971) 10-150 X 0.858 Allkofer et al (1968) 20-1000 X 1. Table 1.…”
Section: Momentum Spectra At the Vertical Directionmentioning
confidence: 99%
“…As these papers are normalized [27] 10/6 0.822 ± 0.009 0.818 ± 0.007 Kremer 1997 data [27] 13/6 0.831 ± 0.008 0.821 ± 0.007 Table 1: Normalization of datasets with respect to the Bugaev calculation to Rossi [28] we recalculate this normalization point with the reference shape. The data of [21] are normalized to the differential flux at 10 GeV/c. The results of this calculation are shown in the last column of table 1.…”
Section: The Shape Of the Muon Spectrummentioning
confidence: 99%