Stability of the solar neutrino flux derived from SAGE data

Details Stability of the solar neutrino flux derived from SAGE data Stability of the solar neutrino flux derived from SAGE data

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009arep...53..166k&link_type=abstract

Astronomy Reports, Volume 53, Issue 2, pp.166-172

Astronomy and Astrophysics

Astronomy

2

95.85.Ry, 96.60.Jw

Scientific paper

To first approximation, the SAGE data indicate that the solar neutrino flux is constant and displays a single-mode distribution. A more detailed analysis shows that the first two years of data (1990-1992) display a stronger scatter of the neutrino flux than do the following years. We discuss possible astronomical implications of this result.

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