The Soviet-American gallium-germanium experiment on the detection of solar neutrinos

Details The Soviet-American gallium-germanium experiment on the detection of solar neutrinos The Soviet-American gallium-germanium experiment on the detection of solar neutrinos

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989izssr..53..355a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Computer Science

Particle Telescopes, Radiation Measurement, Solar Neutrinos, Gallium Isotopes, Germanium Isotopes, International Cooperation, Test Facilities

Scientific paper

The Soviet-American gallium-germanium (GG) experiment on solar-neutrino detection will be carried out at the Baksan neutrino observatory. The GG neutrino telescope is situtated 3500 meters below ground. The system with 30 tons of gallium is ready for operation and it is expected that the first results will be obtained in 1989; after a year of measurements the results are expected to have a statistical reliability of 18 percent; the complete 60-ton system is expected to be fully operational by the end of 1989. In addition, it is expected that the instrumentation for a calibration experiment with an artificial neutrino source (Cr-51) will be completed in 1989.

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