Inside the Sun pp 179-186 | Cite as

The Kamiokande Solar Neutrino Experiment

  • M. Nakahata
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 159)

Abstract

The observation of 8B solar Neutrinos in the Kamiokande-II detector is presented. Based on 450 days of data in the time period of January 1987 through May 1988, the measured flux obtained with Ee ≥ 9.3 MeV was 0.46 ± 0.13 (stat) ± 0.08 (sys) of the value predicted by the standard solar model. The detector and analysis methods were improved since June 1988 and the background level has been decreased by a factor of about three since then.

Keywords

Solar Neutrino Cherenkov Light Standard Solar Model Solid Histogram Solar Neutrino Flux 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • M. Nakahata
    • 1
  1. 1.Institute for Cosmic Ray ResearchUniversity of TokyoTanashi, TokyoJapan

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