A study of atmospheric neutrinos with the IMB detector

Details A study of atmospheric neutrinos with the IMB detector A study of atmospheric neutrinos with the IMB detector

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..116l&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 116-119 (SEE N85-36066 24-93)

Physics

Cosmic Ray Showers, Decay, Neutrinos, Nucleons, Particle Emission, Particle Interactions, Point Sources, Cerenkov Counters, Earth Atmosphere, Flux, Geomagnetism, Oscillations, Radiation Measuring Instruments, Size Distribution

Scientific paper

A sample of 401 contained neutrino interactions collected in the 3300 metric ton fiducial mass IMB detector was used to study neutrino oscillations, geomagnetic modulation of the flux and to search for point sources. The majority of these events are attributed to neutrino interactions. For the most part, these neutrinos are believed to originate as tertiary products of cosmic ray interactions in the atmosphere. The neutrinos are a mixture of ve and v sub micron.

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