1965
DOI: 10.1007/bf02721030
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The momentum spectrum and charge ratio of μ-mesons at sea-level-II

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1967
1967
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Cited by 23 publications
(3 citation statements)
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“…Up to this date, several authors have derived the analytical expressions for the differential atmospheric muon spectra in the reaction between primaries and atmospheric nuclei (Bull et al, 1965;Matsuno et al, 1984;Bugaev et al, 1998;Gaisser and Stanev, 2008). The parameters in their models have been adjusted by comparing these with the observed spectrum of muons taken from experiments made at sea level (Jokisch et al, 1979;Matsuno et al, 1984;Allkofer et al, 1985;Haino et al, 2004;Achard et al, 2004).…”
Section: Cosmic-ray Muonsmentioning
confidence: 99%
“…Up to this date, several authors have derived the analytical expressions for the differential atmospheric muon spectra in the reaction between primaries and atmospheric nuclei (Bull et al, 1965;Matsuno et al, 1984;Bugaev et al, 1998;Gaisser and Stanev, 2008). The parameters in their models have been adjusted by comparing these with the observed spectrum of muons taken from experiments made at sea level (Jokisch et al, 1979;Matsuno et al, 1984;Allkofer et al, 1985;Haino et al, 2004;Achard et al, 2004).…”
Section: Cosmic-ray Muonsmentioning
confidence: 99%
“…A significant amount of data related to the energy spectrum of muons has been accumulated over the past 50 years 16 18 ) and the spectrum has been modeled. 19 22 )…”
Section: Principles Of Muographymentioning
confidence: 99%
“…Primary cosmic rays reacting with the nitrogen and oxygen nuclei at the top of Earth's atmosphere produce mostly pions, which subsequently decay via the process represented as π (pion) → μ (muon) + ν (neutrino). Because of this simple two-body reaction chain, the zenith-angle energy spectrum of muons can be accurately predicted (Bull et al 1965, Matsuno et al 1984, Bugaev et al 1998, Gaisser & Stanev 2008. In the vicinity of Earth, primary cosmic rays arrive isotropically, and the initial information about the course they took to arrive from the source (e.g., a supernova) is completely lost, hence the azimuthal distribution of resultant muons.…”
Section: Principlementioning
confidence: 99%