A. Hawthorne

TL;DR: In this article, a measurement of the flux of neutrino-induced upgoing muons ( ν >∼ 100 GeV) using the MACRO detector is presented, where the ratio of the observed to expected events integrated over all zenith angles is 0.74 ± 0.036 (stat) ±0.13 (theoretical).

TL;DR: An analysis of systematic uncertainties introduced by the interaction models in the atmosphere and the underground propagation of muons is presented and a comparison of results with published data is also presented.

TL;DR: In this article, the authors search for a correlation between variations in the underground muon rate, Nμ, and seasonal temperature variation in the atmosphere with high statistical significance and find that these correlations are present with high significance.

TL;DR: In this paper, the first measurement of the flux of upgoing muons resulting from interactions of atmospheric neutrinos in the rock below MACRO is reported, which is consistent with no neutrino oscillations or some possible oscillation hypothese with the parameters suggested by the Kamiokande contained-event analysis.

TL;DR: MACRO as discussed by the authors was an experiment that ran in the Laboratori Nazionali del Gran Sasso from 1988 to 2000, and its principal goal was to observe magnetic monopoles or set significantly lower experimental flux limits than had been previously available in the velocity range from about beta = 10(-4) to unity.