KAMIOKANDE results on solar neutrinos and a supernova search

Details KAMIOKANDE results on solar neutrinos and a supernova search KAMIOKANDE results on solar neutrinos and a supernova search

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992stia...9344876s&link_type=abstract

International Symposium on Neutrino Astrophysics, Takayamal Kamioka, Japan, Oct. 19-22, 1992, Paper, 11 p.

Astronomy and Astrophysics

Astrophysics

Radiation Detectors, Solar Cycles, Solar Neutrinos, Spectroheliographs, Supernovae, Antineutrinos, Particle Flux Density, Solar Magnetic Field

Scientific paper

The solar neutrino measurement extended till the end of August in 1992 gives almost entire coverage of the solar maximum in solar cycle 22. The observation shows the almost constant solar B-8-neutrino flux of Data/SSM = 0.49 +/- 0.04 +/- 0.06 on an average for the Kamiokande II and III data. The flux limit of the Hep neutrino is shown at first time. A stringent limit on solar anti-neutrinos that is less than 5.8 percent of the flux of B-8 neutrinos is obtained. A search for supernova neutrinos in the Kamiokande detector is briefly summarized and galactic supernova rate obtained is less than 0.54 SN/year for 4.26 years of observation.

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