Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Solar-cycle modulation of event rates in the chlorine solar neutrino experiment

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/169856· OSTI ID:5732499
;  [1]
  1. Institute for Advanced Study, Princeton, NJ (USA) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
The time dependence of the event rates in the Homestake chlorine solar neutrino experiment are reexamined using new Ar-37 production data covering the period from late 1986 to mid-1989. The data span almost two complete solar cycles. A careful statistical analysis using nonparametric rank-order statistics is used to calculate quantitative significance levels that do not depend on experimental errors. The results show that the Ar-37 production rate in the experiment is anticorrelated with solar activity for approximately 1977-1989. The shape of the Ar-37 production rate is different from the inverted sunspot activity curve. The Ar-37 production rate is better descrbed by a skewed sawtooth function than by the sunspot number. The best-fitting sawtooth function with sunspot period has a slow rise and a rapid decline. The Ar-37 maximum occurs about 12.5 yr after the solar sunspot minimum, while minimum Ar-37 production is more nearly simultaneous with the sunspot maximum. 42 refs.
OSTI ID:
5732499
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 370; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English