scholarly journals Characterization of plastic scintillator tiles equipped with SiPMs for the High Energy cosmic-Radiation Detection (HERD) experiment

2019 ◽  
Author(s):  
Fabio Gargano ◽  
A. De Benedittis ◽  
F. Palma ◽  
P. delaTorre Luque ◽  
M. Di Santo ◽  
...  
2019 ◽  
Vol 209 ◽  
pp. 01034
Author(s):  
Vincenzo Vitale

The core of the High-Energy Particle Detector (HEPD) on board of the China Seismo-Electromagnetic Satellite (CSES) is a segmented calorimeter, which is composed with an upper tower of plastic scintillator counters and a bottom array of LYSO large crystals. Electrons with energy below 100MeV, protons and light nuclei, below few hundreds ofMeV/nucleon are fully contained within this calorimeter. Mainly the LYSO array (density 7.3 g/cm3, thickness around 29.2 g/cm2) extends the HEPD energy range, allowing those measurements (solar energetic particles, low-energy cosmic rays) which are more related to astroparticle physics topics. Two identical copies of HEPD, and then of its calorimeter, exist: the Flight (FM) and the Qualification (QM) models. While the FM has achieved the orbit on board of the CSES satellite in February 2018, the Qualification Model, is used, at ground, for tests and calibrations. A report on the characterization of this compact particle space detector and on preliminary studies and results, will be given.


2017 ◽  
Author(s):  
Yongwei Dong ◽  
Ming Xu ◽  
Zhigang Wang ◽  
Oscar Adriani ◽  
Sebastiano Albergo ◽  
...  

2017 ◽  
Vol 1 (1) ◽  
Author(s):  
Zheng Quan ◽  
Zhigang Wang ◽  
Ming Xu ◽  
Yongwei Dong ◽  
Junjing Wang ◽  
...  

Radiocarbon ◽  
1983 ◽  
Vol 25 (3) ◽  
pp. 908-918 ◽  
Author(s):  
J M Punning ◽  
R Rajamäe ◽  
Kai Joers ◽  
H Putnik

This list comprises age measurements carried out at the Institute from 1979 to 1981. Anticoincidence variant was applied to attain higher counting efficiency of a 2-channel scintillation device. The introduction of a plastic scintillator as an active guard around the detector in the 2π geometry decreases the influence of high energy cosmic radiation and reduces the background ca 35 to 75% (Rajamäe & Punning, 1980). The application of an active guard with 4π geometry has proved most effective; as a result, the background decreased 85% to 0.65cpm with the volume of scintillation cocktail 5ml. We have improved our methods for decreasing the actual error of the background. The application of a control channel and consideration of barometric effect results in the increase of dating limits of up to 5000–6000 years (Rajamäe, 1981). Samples are calculated using a half-life of 5568 ± 30 years for 14C. Results are reported in years before 1950. δ13C measurements were performed on the mass-spectrometer MI-1201 and are reported with PDB as a reference standard. The reproducibility of results is ±0.2‰.


2013 ◽  
Author(s):  
Krishna C. Mandal ◽  
Abhinav Mehta ◽  
Sandeep K. Chaudhuri ◽  
Yunlong Cui ◽  
Michael Groza ◽  
...  

2017 ◽  
Author(s):  
Shuang-Nan Zhang ◽  
Oscar Adriani ◽  
Herd Consortium ◽  
Sebastiano Albergo ◽  
Giovanni Ambrosi ◽  
...  

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