Kudryavtsev M I, Bogomolov A V, Bogomolov V V, Svertilov S I
Space Research Institute, Russian Academy of Science, Moscow, Russia.
Adv Space Res. 1998;21(12):1785-8. doi: 10.1016/s0273-1177(98)00067-2.
The measurements of high-energy neutron (with energies approximately 30-300 MeV) and proton (with energies approximately 1-200 MeV) fluxes are being conducted on-board "Mir-Spectr" orbital complex. Neutrons are detected by the undirected (FOV approximately 4 pi sr) scintillator spectrometer, consisting of 4 identical CsI(T1) detector units (the effective area for neutrons approximately 30 cm2). The gamma-quanta, which can be also detected by this instrument, are separated from neutrons by the analysis of the scintillator output pulse shape. To exclude registration of charged particles an anticoincidence plastic scintillator shield is realized in each detector unit. The proton fluxes are measured by the telescope based on 3 semiconductor detectors with small geometry factor (approximately 1 cm2 x sr). As the first result of the experiment the upper limit of the integral flux of local and albedo neutrons in the equatorial region (L<1. 1) was estimated. The results of this measurements can be useful for the radiation security. Also, the neutrons of solar flares can be detected in this experiment.
在“和平号 - 光谱”轨道综合体上正在进行高能中子(能量约为30 - 300兆电子伏特)和质子(能量约为1 - 200兆电子伏特)通量的测量。中子由无定向(视场约4π球面度)闪烁体光谱仪探测,该光谱仪由4个相同的碘化铯(铊)探测器单元组成(中子的有效面积约为30平方厘米)。该仪器也能探测到的伽马量子,通过分析闪烁体输出脉冲形状与中子分离。为排除带电粒子的记录,在每个探测器单元中设置了反符合塑料闪烁体屏蔽。质子通量由基于3个小几何因子(约1平方厘米×球面度)半导体探测器的望远镜测量。作为实验的首个结果,估算了赤道区域(L < 1.1)本地和反照中子积分通量的上限。这些测量结果对辐射安全可能有用。此外,在该实验中还能探测到太阳耀斑的中子。