论文标题
用两个hisparc闪烁器探测$ 10^{12} $ 10^{12} $的宇宙射线能量
Probing the cosmic ray energy spectrum at $10^{12}$--$10^{16}$ eV with two HiSPARC scintillators
论文作者
论文摘要
宇宙天体物理学研究的高中项目（HISPARC）采用了大量的小型探测站，这些探测站对广泛的宇宙射线空中阵雨进行了品尝。这些电台中的大多数都有两个0.5 \ si {\ meter \ squared}闪烁检测器。提出了一种新方法，该方法可以在五十年中使用一个两阶尺的宇宙射线通量探测$ 10^{12} $，$ 10^{13} $，$ 10^{14} $，$ 10^{15} $，$ 10^{15} $和$ 10^{16} $ ev。该方法基于通过单个检测器的粒子数量的分布的能量依赖性。相对较短的数据花费大约一个月足以探测此能量范围。通量值与其他实验的测量非常吻合。 $ 10^{12} $的宇宙射线通量和$ 10^{13} $ eV是在海平面衍生的。
The high school project on astrophysics research with cosmics (HiSPARC) employs a large number of small detection stations that sample the footprint of extensive cosmic ray air showers. The majority of these stations has two 0.5 \si{\meter\squared} scintillation detectors. A new method is presented which enables probing the cosmic ray flux with a single two-scintillator station in five energy decades at $10^{12}$, $10^{13}$, $10^{14}$, $10^{15}$ and $10^{16}$ eV. The method is based on the energy dependence of the distribution of the number of particles passing through a single detector. A relatively short data taking period of approximately one month is sufficient to probe this energy range. The flux values agree well with measurements by other experiments. For the first time, the cosmic ray flux at $10^{12}$ and $10^{13}$ eV is derived at sea level.
