论文标题
太阳中微子作为太阳活动的指标
Solar neutrinos as indicators of the Sun's activity
论文作者
论文摘要
研究了太阳耀斑（SF）预测的机会，观察了太阳中微子通量。在三个中微子的世代中，中微子通量的演变被认为是SF源的耦合黑子（CS）。假定中微子既具有偶极磁矩，又具有Anapole矩，而CS上方的磁场可能达到$ 10^5-10^6 $ GS的值，显示扭曲性质并具有非电位特征。检查了太阳中微子通量的可能共振转换。由于$ν_{el} \至ν_{μl} $共振发生在对流区域之前，因此其存在绝不可以与SF连接。但是，当太阳中微子通量在预段期间穿过CS时，它可能会经历其他共振转化率，因此，可以观察到电子中微子通量耗尽。
Opportunity of the solar flares (SF's) prediction observing the solar neutrino fluxes is investigated. In three neutrino generations the evolution of the neutrino flux traveling the coupled sunspots (CS's) which are the SF source is considered. It is assumed that the neutrinos possess both the dipole magnetic moment and the anapole moment while the magnetic field above the CS's may reach the values $10^5-10^6$ Gs, displays the twisting nature and has the nonpotential character. The possible resonance conversions of the solar neutrino flux are examined. Since the $ν_{eL}\to ν_{μL}$ resonance takes place before the convective zone, its existence can in no way be connected with the SF. However, when the solar neutrino flux moves through the CS's in the preflare period, then it may undergo the additional resonance conversions and, as a result, depleting the electron neutrinos flux may be observed.
