Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1391r&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
We have studied solar neutrino flux data from super-Kamiokande(SK), SAGE, GALLEX-GNO detectors statistically and have shown that solar neutrino flux data varies with the solar activity cycle.We have also studied the solar neutrino flux data during the period from 31May 1996 to 31December 2001 from SAGE,GNO and superkamiokande detectors we find 5 and 10 months in the solar neutrino flux data with more than 99% C.L. and 5 months period have already been observed in solar neutrino flux data from Homestake detector,sunspot data,solar proton events data etc.which indicates that solar activity cycle is due to the pulsating character of nuclear energy generation inside the sun.For the strength of our suggestion we have studied the fractal nature of solar interior along with solar flares,sunspot data and we find that both the solar neutrino flux data and solar surface data (i.e.,sunspot data,solar flares data etc.) are fractal in nature. All the observed fact and short time variation indicate that the standard solar model must be modified to include the variable nature of solar interior.
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