Solar flares and neutrino detectors.
Solar flares and neutrino detectors.
复制标题
太阳耀斑和中微子探测器。
作者：
Bahcall
在太阳中微子实验中，太阳耀斑被认为是偶然的高计数率的原因。评价了中微子探测器对耀斑的灵敏度。如果在氯实验中探测到耀斑，那么当电磁观测到显著的耀斑时，几个中微子探测器将显示出大的信号。
Solar flares have been suggested as the cause of occasional high counting rates in the $^{37}\mathrm{Cl}$ solar-neutrino experiment. The sensitivity of neutrino detectors to flares is evaluated. Several neutrino detectors will show large signals when prominent flares are observed electromagnetically, if flares are detected in the chlorine experiment.