The High Energy Cosmic Radiation Detection (HERD) facility is a dedicated particle astrophysics experiment planned to be installed on China's Space Station. The Silicon Charge Detector (SCD), one of the sub-detectors of HERD, is designed to measure the charge of cosmic-ray nuclei with atomic numbers from Z = 1 to 28. The full-scale SCD detector module has been successfully developed for the first time. This paper presents the assembly of the detector module, as well as its performance evaluated through laser and beam tests.

Performance characterization of full-scale detector module for HERD silicon charge detector / Long H.-Y., Li H.-Y., Qiao R., Wei J.-J., Gong K., Lan X.-F., Peng W.-X., Lu B., Xiong J.-J., Guo D.-Y., Liu Y.-Q., Wang Z.-G., Wang R.-J., Dong Y.-W., Guo J.-H., Adriani O., Berti E., Betti P., Casaus J., Detti S., et al.. - In: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT. - ISSN 0168-9002. - ELETTRONICO. - 1089:(2026), pp. 1-0. (2017 European Physical Society Conference on High Energy Physics ) [10.1016/j.nima.2026.171559].

Performance characterization of full-scale detector module for HERD silicon charge detector

Adriani O.;Berti E.;Betti P.;Martinez G.;Pacini L.;Tiberio A.;Scaringella M.;Starodubtsev O.;Zampa G.;
2026

Abstract

The High Energy Cosmic Radiation Detection (HERD) facility is a dedicated particle astrophysics experiment planned to be installed on China's Space Station. The Silicon Charge Detector (SCD), one of the sub-detectors of HERD, is designed to measure the charge of cosmic-ray nuclei with atomic numbers from Z = 1 to 28. The full-scale SCD detector module has been successfully developed for the first time. This paper presents the assembly of the detector module, as well as its performance evaluated through laser and beam tests.
2026
Proceedings of Science
2017 European Physical Society Conference on High Energy Physics
Long H.-Y.; Li H.-Y.; Qiao R.; Wei J.-J.; Gong K.; Lan X.-F.; Peng W.-X.; Lu B.; Xiong J.-J.; Guo D.-Y.; Liu Y.-Q.; Wang Z.-G.; Wang R.-J.; Dong Y.-W....espandi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1500285
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