2012
DOI: 10.5194/gi-1-185-2012
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Atmospheric muons: experimental aspects

Abstract: Abstract. We present a review of atmospheric muon flux and energy spectrum measurements over almost six decades of muon momentum. Sea level and underground/water/ice experiments are considered. Possible sources of systematic errors in the measurements are examined. The characteristics of underground/water muons (muons in bundle, lateral distribution, energy spectrum) are discussed. The connection between the atmospheric muon and neutrino measurements are also reported.

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Cited by 49 publications
(49 citation statements)
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“…However, theoretically the hard‐muon sea level intensity can be strongly affected by the geomagnetic field from R C about 1 GV depending on the phase factor and energy loss coefficients chosen. In addition, Allkofer et al (), Kremer et al (), Grieder (), and Cecchini and Spurio () and references therein pointed out that the geomagnetic effect is very important even for low‐energy muons at sea level. They found differences in the spectra and differential and integral intensity of low‐energy muons even when comparing data at lower cutoff rigidity (0.5–1 GV) regions.…”
Section: Final Remarksmentioning
confidence: 99%
“…However, theoretically the hard‐muon sea level intensity can be strongly affected by the geomagnetic field from R C about 1 GV depending on the phase factor and energy loss coefficients chosen. In addition, Allkofer et al (), Kremer et al (), Grieder (), and Cecchini and Spurio () and references therein pointed out that the geomagnetic effect is very important even for low‐energy muons at sea level. They found differences in the spectra and differential and integral intensity of low‐energy muons even when comparing data at lower cutoff rigidity (0.5–1 GV) regions.…”
Section: Final Remarksmentioning
confidence: 99%
“…The background such searches have to fight with is mainly due to muons of the cosmic radiation [61] and natural radioactivity. For this reason, different large detectors have been installed in underground laboratories.…”
Section: B Direct Searches In the Cosmic Radiationmentioning
confidence: 99%
“…These can, if energetic enough, experience in turn inelastic interactions with others atoms, or decay into hadrons, photons and leptons. In this scheme, the atmospheric muons (Cecchini and Spurio, 2012) used in tomography are mostly coming from the decays of two kind of hadrons: charged pions and kaons. As pions constitute the most important part of the hadronic component of the showers, and since the charged ones decay almost exclusively into muons, their contribution is dominant.…”
Section: The Physics Of Air Showersmentioning
confidence: 99%