Charge Measurement of Cosmic Ray Nuclei with the Plastic Scintillator Detector of DAMPE
arXiv:1810.10784 · doi:10.1016/j.astropartphys.2018.10.001
Abstract
One of the main purposes of the DArk Matter Particle Explorer (DAMPE) is to measure the cosmic ray nuclei up to several tens of TeV or beyond, whose origin and propagation remains a hot topic in astrophysics. The Plastic Scintillator Detector (PSD) on top of DAMPE is designed to measure the charges of cosmic ray nuclei from H to Fe and serves as a veto detector for discriminating gamma-rays from charged particles. We propose in this paper a charge reconstruction procedure to optimize the PSD performance in charge measurement. Essentials of our approach, including track finding, alignment of PSD, light attenuation correction, quenching and equalization correction are described detailedly in this paper after a brief description of the structure and operational principle of the PSD. Our results show that the PSD works very well and almost all the elements in cosmic rays from H to Fe are clearly identified in the charge spectrum.
20 pages, 4 figures
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- Observations of Forbush Decreases of cosmic ray electrons and positrons with the Dark Matter Particle Explorer
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- Correction Method for the Readout Saturation of the DAMPE Calorimeter
- Search for relativistic fractionally charged particles in space
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- An Unsupervised Machine Learning Method for Electron--Proton Discrimination of the DAMPE Experiment
- Hadronic cross section measurements with the DAMPE space mission using 20GeV-10TeV cosmic-ray protons and He
- Diverse properties of electron Forbush decreases revealed by the Dark Matter Particle Explorer
- Investigation of hadronic cross sections of cosmic ray carbon and oxygen on BGO from 200 GeV to 10 TeV energy at the DAMPE experiment