机构地区:[1]Institute of Modern Physics, Chinese Academy of Sciences [2]University of Chinese Academy of Sciences [3]Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences [4]School of Astronomy and Space Science, University of Science and Technology of China [5]Istituto Nazionale di Fisica Nucleare (INFN) - Sezione di Lecce [6]Dipartimento di Matematica e Fisica E.De Giorgi, Universit`a del Salento [7]Department of Nuclear and Particle Physics, University of Geneva [8]Gran Sasso Science Institute [9]INFN Laboratori Nazionali del Gran Sasso [10]Department of Modern Physics, University of Science and Technology of China
出 处:《Research in Astronomy and Astrophysics》2019年第3期145-154,共10页天文和天体物理学研究(英文版)
基 金:funded by the National Key Research and Development Program of China (2016YFA0400201);supported by the National Natural Science Foundation of China (11673047,11673075, 11303107, U1738127 and U1738205)
摘 要:The DArk Matter Particle Explorer(DAMPE) is a space-borne apparatus for detecting the highenergy cosmic-ray-like electrons, γ-rays, protons and heavy ions. The Plastic Scintillator Detector(PSD)is the top-most sub-detector of the DAMPE. The PSD is designed to measure the charge of incident highenergy particles and it also serves as a veto detector for discriminating γ-rays from charged particles. In this paper, a PSD on-orbit calibration procedure is described, which includes the five steps of pedestal, dynode correlation, response to minimum-ionizing particles, light attenuation function and energy reconstruction.A method for reconstructing the charge of incident high energy cosmic-ray particles is introduced. The detection efficiency of each PSD strip is verified to be above 99.5%; the total efficiency of the PSD for charged particles is above 99.99%.The DArk Matter Particle Explorer(DAMPE) is a space-borne apparatus for detecting the highenergy cosmic-ray-like electrons, γ-rays, protons and heavy ions. The Plastic Scintillator Detector(PSD)is the top-most sub-detector of the DAMPE. The PSD is designed to measure the charge of incident highenergy particles and it also serves as a veto detector for discriminating γ-rays from charged particles. In this paper, a PSD on-orbit calibration procedure is described, which includes the five steps of pedestal, dynode correlation, response to minimum-ionizing particles, light attenuation function and energy reconstruction.A method for reconstructing the charge of incident high energy cosmic-ray particles is introduced. The detection efficiency of each PSD strip is verified to be above 99.5%; the total efficiency of the PSD for charged particles is above 99.99%.
关 键 词:COSMIC RAY instrumentation: DAMPE charge measurement plastic scintillator detector CALIBRATION
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