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Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout
Recent advances in silicon photomultiplier (SiPM) technology and new scintillator materials allow for the creation of compact high-performance gamma-ray detectors which can be deployed on small low-cost satellites. A small number of such satellites can provide full sky coverage and complement, or in...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Netherlands
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8556215/ https://www.ncbi.nlm.nih.gov/pubmed/34744307 http://dx.doi.org/10.1007/s10686-021-09767-z |
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author | Murphy, David Mangan, Joseph Ulyanov, Alexei Walsh, Sarah Dunwoody, Rachel Hanlon, Lorraine Shortt, Brian McBreen, Sheila |
author_facet | Murphy, David Mangan, Joseph Ulyanov, Alexei Walsh, Sarah Dunwoody, Rachel Hanlon, Lorraine Shortt, Brian McBreen, Sheila |
author_sort | Murphy, David |
collection | PubMed |
description | Recent advances in silicon photomultiplier (SiPM) technology and new scintillator materials allow for the creation of compact high-performance gamma-ray detectors which can be deployed on small low-cost satellites. A small number of such satellites can provide full sky coverage and complement, or in some cases replace the existing gamma-ray missions in detection of transient gamma-ray events. The aim of this study is to test gamma-ray detection using a novel commercially available CeBr(3) scintillator combined with SiPM readout in a near-space environment and inform further technology development for a future space mission. A prototype gamma-ray detector was built using a CeBr(3) scintillator and an array of 16 J-Series SiPMs by ON Semiconductor. SiPM readout was performed using SIPHRA, a radiation-tolerant low-power integrated circuit developed by IDEAS. The detector was flown as a piggyback payload on the Advanced Scintillator Compton Telescope balloon flight from Columbia Scientific Balloon Facility. The payload included the detector, a Raspberry Pi on-board computer, a custom power supply board, temperature and pressure sensors, a Global Navigation Satellite System receiver and a satellite modem. The balloon delivered the detector to 37 km altitude where its detection capabilities and readout were tested in the radiation-intense near-space environment. The detector demonstrated continuous operation during the 8-hour flight and after the landing. It performed spectral measurements in an energy range of 100 keV to 8 MeV and observed the 511 keV gamma-ray line arising from positron annihilation in the atmosphere with full width half maximum of 6.8%. During ascent and descent, the detector count rate peaked at an altitude of 16 km corresponding to the point of maximum radiation intensity in the atmosphere. Despite several engineering issues discovered after the flight test, the results of this study confirm the feasibility of using CeBr(3) scintillator, SiPMs, and SIPHRA in future space missions. |
format | Online Article Text |
id | pubmed-8556215 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | Springer Netherlands |
record_format | MEDLINE/PubMed |
spelling | pubmed-85562152021-11-04 Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout Murphy, David Mangan, Joseph Ulyanov, Alexei Walsh, Sarah Dunwoody, Rachel Hanlon, Lorraine Shortt, Brian McBreen, Sheila Exp Astron (Dordr) Original Article Recent advances in silicon photomultiplier (SiPM) technology and new scintillator materials allow for the creation of compact high-performance gamma-ray detectors which can be deployed on small low-cost satellites. A small number of such satellites can provide full sky coverage and complement, or in some cases replace the existing gamma-ray missions in detection of transient gamma-ray events. The aim of this study is to test gamma-ray detection using a novel commercially available CeBr(3) scintillator combined with SiPM readout in a near-space environment and inform further technology development for a future space mission. A prototype gamma-ray detector was built using a CeBr(3) scintillator and an array of 16 J-Series SiPMs by ON Semiconductor. SiPM readout was performed using SIPHRA, a radiation-tolerant low-power integrated circuit developed by IDEAS. The detector was flown as a piggyback payload on the Advanced Scintillator Compton Telescope balloon flight from Columbia Scientific Balloon Facility. The payload included the detector, a Raspberry Pi on-board computer, a custom power supply board, temperature and pressure sensors, a Global Navigation Satellite System receiver and a satellite modem. The balloon delivered the detector to 37 km altitude where its detection capabilities and readout were tested in the radiation-intense near-space environment. The detector demonstrated continuous operation during the 8-hour flight and after the landing. It performed spectral measurements in an energy range of 100 keV to 8 MeV and observed the 511 keV gamma-ray line arising from positron annihilation in the atmosphere with full width half maximum of 6.8%. During ascent and descent, the detector count rate peaked at an altitude of 16 km corresponding to the point of maximum radiation intensity in the atmosphere. Despite several engineering issues discovered after the flight test, the results of this study confirm the feasibility of using CeBr(3) scintillator, SiPMs, and SIPHRA in future space missions. Springer Netherlands 2021-06-25 2021 /pmc/articles/PMC8556215/ /pubmed/34744307 http://dx.doi.org/10.1007/s10686-021-09767-z Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Original Article Murphy, David Mangan, Joseph Ulyanov, Alexei Walsh, Sarah Dunwoody, Rachel Hanlon, Lorraine Shortt, Brian McBreen, Sheila Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout |
title | Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout |
title_full | Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout |
title_fullStr | Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout |
title_full_unstemmed | Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout |
title_short | Balloon flight test of a CeBr(3) detector with silicon photomultiplier readout |
title_sort | balloon flight test of a cebr(3) detector with silicon photomultiplier readout |
topic | Original Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8556215/ https://www.ncbi.nlm.nih.gov/pubmed/34744307 http://dx.doi.org/10.1007/s10686-021-09767-z |
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