Time Variations of the Superkamiokande Solar Neutrino Flux Data 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 the Rayleigh Power Spectrum Analysis of the solar neutrino flux data from 1) 5-day-long samples from Super-Kamiokande-I detector during the period from June, 1996 to July, 2001; 2) 10 -day-long samples from the same detector during the same period and (3) 45-day long from the same detector during the same period. According to our analysis (1) gives periodicities around 0.25, 23.33, 33.75 and 42.75 months; (2) exhibits periodicities around 0.5, 1.0, 28.17, 40.67 and 52.5 months and (3) shows periodicities around 16.5 and 28.5 months. We have found almost similar periods in the solar flares, sunspot data, solar proton data.
dc.description4 pages including 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0606082
dc.identifierhttp://arxiv.org/abs/astro-ph/0606082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111973
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTime Variations of the Superkamiokande Solar Neutrino Flux Data by Rayleigh Power Spectrum Analysis
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