MHD solar fluctuations and solar neutrinos

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8348

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DC Field	Value	Language
dc.creator	Reggiani N.	-
dc.creator	Guzzo M.M.	-
dc.creator	Holanda P.C. de	-
dc.date	2003	-
dc.date.accessioned	2013-06-01T10:55:09Z	-
dc.date.available	2013-06-01T10:55:09Z	-
dc.date.issued	2013-06-01	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332003000400028	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2003&volume=33&issue=4&spage=707	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/8348	-
dc.description	We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamic (MHD) perturbations of the solar plasma. We state that if such time fluctuations are detected, this would provide a unique signature of the Resonant Spin-Flavor Precession (RSFP) mechanism as a solution to the Solar Neutrino Problem.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	MHD solar fluctuations and solar neutrinos	-
Appears in Collections:	Physics and Astronomy

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