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New narrow-beam neutron spectrometer in complex monitoring system

机译:复杂监测系统中的新型窄束中子光谱仪

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In the interaction of cosmic rays (CRs) with Earth’s atmosphere, neutrons are formed in a wide range of energies: from thermal (E≈0.025 eV) to ultrarelativistic (E1 GeV). To detect and study CRs, Polar Geophysical Institute (PGI) uses a complex monitoring system containing detectors of various configurations. The standard neutron monitor (NM) 18-NM-64 is sensitive to neutrons with energies E50 MeV. The lead-free section of the neutron monitor (BSRM) detects neutrons with energies E≈(0.1÷1) MeV. Also, for sharing with standard detectors, the Apatity NM station has developed and installed a neutron spectrometer with three energy channels and a particle reception angle of 15 degrees. The configuration of the device makes it possible to study the degree of anisotropy of the particle flux from different directions. We have obtained characteristics of the detector (response function and particle reception angle), as well as geometric dimensions through numerical simulation using the GEANT4 toolkit [Agostinelli et al., 2003]. During operation of the device, we collected database of observations and received preliminary results.
机译:在宇宙射线(CR)与地球大气层的相互作用中,中子形成的能量范围很广:从热能(E≈0.025eV)到超相对论(E> 1 GeV)。为了检测和研究CR,极地地球物理研究所(PGI)使用了一个复杂的监视系统,其中包含各种配置的探测器。标准中子监测器(NM)18-NM-64对能量E> 50 MeV的中子敏感。中子监测器(BSRM)的无铅部分检测能量为E≈(0.1÷1)MeV的中子。另外,为了与标准探测器共享,Apatity NM站开发并安装了具有三个能量通道和15度粒子接收角的中子光谱仪。该装置的构造使得有可能研究来自不同方向的粒子通量的各向异性程度。通过使用GEANT4工具包进行的数值模拟,我们已经获得了检测器的特性(响应函数和粒子接收角度)以及几何尺寸[Agostinelli等,2003]。在设备运行期间,我们收集了观测数据库并收到了初步结果。

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