The chlorine solar neutrino experiment

Details The chlorine solar neutrino experiment The chlorine solar neutrino experiment

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aipc..126....1r&link_type=abstract

IN: Solar neutrinos and neutrino astronomy; Proceedings of the Conference, Lead, SD, August 23-25, 1984 (A86-37626 17-93). New Y

Astronomy and Astrophysics

Astronomy

57

Chlorine, Radiation Measuring Instruments, Solar Activity, Solar Neutrinos, Argon Isotopes, Background Radiation, Monte Carlo Method, Proton-Proton Reactions, Solar Flares

Scientific paper

The present consideration of the fourteen years' (1970-1984) results from the Homestake Gold Mine chlorine solar neutrino experiment gives attention to background processes generating Ar-37, as well as the constancy of the Ar-37 production rate. The counter background rates derived from a maximum likelihood treatment are noted to have been variable. The results of the chlorine experiment are clearly different from those of Monte Carlo simulations, with a production rate 3-4 times higher. Solar cycle variations and solar flare effects are also discussed.

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