Solar MHD Waves and Solar Neutrinos

被引：0
|
作者：
N. Reggiani
M.M. Guzzo
P.C. de Holanda
机构：
[1] Universidade Católica de Campinas,Faculdade de Matemática, Centro de Ciências Exatas Ambientais e de Tecnologias, Pontifí cia
[2] Instituto de Fí sica Gleb Wataghin,undefined
[3] Universidade Estadual de Campinas,undefined
[4] The Abdus Salam International Centre for Theoretical Physics,undefined
来源：
Space Science Reviews | 2003年 / 107卷
关键词：
magnetic perturbations; neutrino; oscillation;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We analyze here how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamics (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.
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页码：89 / 97
页数：8
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