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Observation of muon intensity variations by season with the MINOS Near Detector

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arxiv 1406.7019 v1 pith:R3HIJAMA submitted 2014-06-26 hep-ex astro-ph.IMphysics.ins-det

classification hep-exastro-ph.IMphysics.ins-det
keywords muontemperatureeffectivechangecoefficientdetectordeterminedminos
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abstract

A sample of 1.53$\times$10$^{9}$ cosmic-ray-induced single muon events has been recorded at 225 meters-water-equivalent using the MINOS Near Detector. The underground muon rate is observed to be highly correlated with the effective atmospheric temperature. The coefficient $\alpha_{T}$, relating the change in the muon rate to the change in the vertical effective temperature, is determined to be 0.428$\pm$0.003(stat.)$\pm$0.059(syst.). An alternative description is provided by the weighted effective temperature, introduced to account for the differences in the temperature profile and muon flux as a function of zenith angle. Using the latter estimation of temperature, the coefficient is determined to be 0.352$\pm$0.003(stat.)$\pm$0.046(syst.).

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Monitoring the upper atmospheric temperature and interplanetary magnetic field with the GRAPES-3 muon telescope

    astro-ph.HE 2026-02 conditional novelty 4.0 of 10

    From 22 years of GRAPES-3 muon data, the temperature response is -0.224 ± 0.022 %/K and the interplanetary magnetic-field response is -0.574 ± 0.011 %/nT, giving the telescope a possible proxy-monitoring role.

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