Possibility of parametrization of atmospheric muon angular flux using underwater data

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dc.creatorKlimushin, S. I.
dc.creatorBugaev, E. V.
dc.creatorSokalski, I. A.
dc.date2002-02-07
dc.date.accessioned2026-07-07T03:46:28Z
dc.date.available2026-07-07T03:46:28Z
dc.descriptionWe present the formula for angular distribution of integral flux of conventional ($π, K$) muons deep under water taking into account the sphericity of the atmosphere and fluctuations of muon energy losses.The accuracy of this formula for various sea level muon spectra is discussed. The possibility of reconstructing two parameters of sea level spectrum by fitting measured underwater angular intensity is shown for Baikal Neutrino Telescope NT--36 experimental data.
dc.descriptionContribution to the Proc. of 2nd Workshop on Methodical Aspects of Underwater/Underice Neutrino Telescopes, Hamburg, August 15-16, 2001, 6 pages, 7 .eps figures, uses nuws.cls
dc.identifierhttps://arxiv.org/abs/hep-ph/0202065
dc.identifierhttp://arxiv.org/abs/hep-ph/0202065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41303
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePossibility of parametrization of atmospheric muon angular flux using underwater data
dc.typetext

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