Time Variations of the Solar Neutrino Flux Data from Sage and Gallex-Gno Detectors Obtained by Rayleigh Power Spectrum Analysis

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dc.creatorGhosh, Koushik
dc.creatorRaychaudhuri, Probhas
dc.date2006-06-05
dc.date.accessioned2026-07-07T07:12:07Z
dc.date.available2026-07-07T07:12:07Z
dc.descriptionWe have used Rayleigh power spectrum analysis of the monthly solar neutrino flux data from (1) SAGE detector during the period from 1st January 1990 to 31st December 2000; (2) SAGE detector during the period from April 1998 to December 2001; (3) GALLEX detector during the period from May 1991 to January 1997; (4) GNO detector during the period from May 1998 to December 2001; (5) GALLEX-GNO detector (combined data) from May 1991 to December 2001 and (6) average of the data from GNO and SAGE detectors during the period from May 1998 to December 2001. (1) exhibits periodicity around 1.3, 4.3, 5.5, 6.3, 7.9, 8.7, 15.9, 18.7, 23.9, 32.9 and 48.7 months. (2) shows periodicity around 1.5, 2.9, 4.5, 10.1 months. For (3) we observe periodicity around 1.7, 18.7 and 26.9 months. For (4) periodicity is seen around 3.5, 5.5, 7.7 and 10.5 months. (5) gives periodicity around 1.7, 18.5, 28.5 and 42.1 months while (6) shows periodicity around 4.3, 6.9, 10.3 and 18.1 months. We have found almost similar periods in the solar flares, sunspot data, solar proton data which indicates that the solar activity cycle may be due to the variable character of nuclear energy generation inside the sun.
dc.description4 pages including 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0606083
dc.identifierhttp://arxiv.org/abs/astro-ph/0606083
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111974
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTime Variations of the Solar Neutrino Flux Data from Sage and Gallex-Gno Detectors Obtained by Rayleigh Power Spectrum Analysis
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