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A measurement is presented of the flux ratio of positive and negative muons from cosmic ray interactions in the atmosphere, using data collected by the CMS detector at ground level and in the underground experimental cavern. The excellent…

High Energy Physics - Experiment · Physics 2011-04-22 Lars Sonnenschein

This paper describes a new measurement of the flux ratio of positive and negative muons from cosmic-ray interactions in the atmosphere, using data collected by the CMS detector at ground level and in the underground experimental cavern. The…

High Energy Physics - Experiment · Physics 2010-10-07 Gavin Hesketh

We present a measurement of the ratio of positive to negative muon fluxes from cosmic ray interactions in the atmosphere, using data collected by the CMS detector both at ground level and in the underground experimental cavern at the CERN…

High Energy Physics - Experiment · Physics 2012-08-27 The CMS Collaboration

The absolute muon flux between 20 GeV and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degree. Due to the large exposure of about 150 m2 sr d, and the excellent momentum…

High Energy Physics - Experiment · Physics 2012-08-27 The L3 Collaboration

The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon intensities at depths up to 18 km w.e. are calculated. The results are particularly collated with a great body of the ground-level,…

High Energy Physics - Phenomenology · Physics 2014-11-17 E. V. Bugaev , A. Misaki , V. A. Naumov , T. S. Sinegovskaya , S. I. Sinegovsky , N. Takahashi

The atmospheric muon spectrum between 20 and 2000 GeV was measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 to 58 degrees. Due to the large data set and the good detector resolution, a precision of 2.6% at 100…

High Energy Physics - Experiment · Physics 2019-08-14 Michael Unger

We present a new measurement of air shower muons made during atmospheric ascent of the High Energy Antimatter Telescope balloon experiment. The muon charge ratio mu+ / mu- is presented as a function of atmospheric depth in the momentum…

The ALEPH detector at LEP has been used to measure the momentum spectrum and charge ratio of vertical cosmic ray muons underground. The sea-level cosmic ray muon spectrum for momenta up to 2.5 TeV/c has been obtained by correcting for the…

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…

Earth and Planetary Astrophysics · Physics 2012-08-16 Stefano Cecchini , Maurizio Spurio

In this paper we discuss the problem, why the use of the direct data on primary nuclei spectra together with the modern hadronic interaction models leads to significant deficit of computed vertical muon flux at sea level for energies $>100$…

Astrophysics · Physics 2009-11-10 A. A. Lagutin , A. G. Tyumentsev , A. V. Yushkov

The magnetized MINOS near detector can accurately determine the charge sign of atmospheric muons, this facilitates a measurement of the atmospheric muon charge ratio. To reduce the systematic error associated with geometric bias and…

High Energy Physics - Experiment · Physics 2019-08-13 J. K. de Jong

We report measurements of the angular distributions of low momentum atmospheric muons at 38 m above sea level for zenith angles $\theta$ between -60 and 60 degrees in the south-north direction. The muon detection was performed with two…

Instrumentation and Detectors · Physics 2023-04-14 Issa Briki , Malek Mazouz , Lotfi Ghedira

We present a new measurement of atmospheric muons made during an ascent of the High Energy Antimatter Telescope balloon experiment. The muon charge ratio mu+/mu- as a function of atmospheric depth in the momentum interval 0.3-0.9 GeV/c is…

Atmospheric neutrino-fluxes are calculated over the wide energy range from 30 MeV to 3,000 GeV for the study of neutrino-physics using the data from underground neutrino-detectors. The atmospheric muon-flux at high altitude and at sea level…

High Energy Physics - Phenomenology · Physics 2009-10-28 M. Honda , T. Kajita , S. Midorikawa , K. Kasahara

In the near future the energy region above few hundreds of TeV may really be accessible for measurements of the atmospheric muon spectrum by the IceCube array. Therefore one expects that muon flux uncertainties above 50 TeV, related to a…

High Energy Astrophysical Phenomena · Physics 2014-11-20 S. I. Sinegovsky , A. A. Kochanov , T. S. Sinegovskaya , A. Misaki , N. Takahashi

We present the measurement of the the flux and angular distribution of atmospheric muon neutrinos using the MACRO detector. Three different event topologies are detected in two different energy ranges. High energy neutrinos (E~80 GeV) via…

High Energy Physics - Experiment · Physics 2009-10-31 M. Spurio

The flux of muons induced by atmospheric neutrinos has been measured with the MACRO detector. Different event topologies have been detected, due to neutrino interactions in the apparatus and in the rock below it. The upward-throughgoing…

High Energy Physics - Experiment · Physics 2007-05-23 Paolo Bernardini

For the first time a complete set of the most recent direct data on primary cosmic ray spectra is used as input into calculations of muon flux at sea level in wide energy range $E_\mu=1-3\cdot10^5$ GeV. Computations have been performed with…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. A. Lagutin , A. G. Tyumentsev , A. V. Yushkov

The vertical absolute fluxes of atmospheric muons and muon charge ratio have been measured precisely at different geomagnetic locations by using the BESS spectrometer. The observations had been performed at sea level (30 m above sea level)…

The analytical expression for angular integral flux of atmospheric muons in matter with the explicit relation of its parameters with those of the sea level spectrum is obtained. The fitting formula for the sea level muon spectrum at…

High Energy Physics - Phenomenology · Physics 2014-11-17 S. I. Klimushin , E. V. Bugaev , I. A. Sokalski
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