Solar neutrino flux variation and its implications

dc.contributor.author	Raychaudhuri, Probhas
dc.date.accessioned	2007-09-17T12:13:17Z
dc.date.available	2007-09-17T12:13:17Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol. 24, No. 2, pp. 143-146	en
dc.identifier.uri	http://hdl.handle.net/2248/1801
dc.description.abstract	Considering the solar neutrino flux data during the period from June 1989 to April 1992 from four solar neutrino experiments (Cl Solar neutrino experiment, SAGE I & II, GALLEX, Kamiokande II & III) we suggest that the solar neutrino flux appears to be varying with the solar activity cycle. The above variation of solar neutrino flux data with the solar activity cycle and the common periodicity around 2.5 years of solar neutrino flux data, solar diameter data, sunspot number data, solar proton events data, Forbush decreases with solar flares data etc., suggests that the pulsating character of the nuclear energy generation inside the solar core may be their common origin.	en
dc.format.extent	387936 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..143R	en
dc.subject	Solar neutrinos	en
dc.title	Solar neutrino flux variation and its implications	en
dc.type	Article	en