Astrophysical Neutrino Telescopes

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dc.creatorMcDonald, A. B.
dc.creatorSpiering, C.
dc.creatorSchoenert, S.
dc.creatorKearns, E. T.
dc.creatorKajita, T.
dc.date2003-11-14
dc.date.accessioned2026-07-07T12:00:58Z
dc.date.available2026-07-07T12:00:58Z
dc.descriptionThis review describes telescopes designed to study neutrinos from astrophysical sources. These sources include the Sun and Supernovae emitting neutrino energies up to tens of MeV, atmospheric neutrino sources caused by cosmic ray interactions and other sources generating neutrino energies ranging up to $1\times 10^{20}$ eV. Measurements with these telescopes also provide information on neutrino properties including clear evidence for neutrino flavor change. Telescopes in operation in the past and present are described, along with plans for future instruments to expand this rapidly growing field of particle astrophysics.
dc.description28 pages, 31 figures, Invited review article submitted to Review of Scientific Instruments May 19, 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0311343
dc.identifierhttp://arxiv.org/abs/astro-ph/0311343
dc.identifierRev.Sci.Instrum.75:293-316,2004
dc.identifierdoi:10.1063/1.1642740
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206959
dc.subjectAstrophysics
dc.titleAstrophysical Neutrino Telescopes
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