Slawomir Mianowski, Nicolas De Angelis, Johannes Hulsman, Merlin Kole, Tomasz Kowalski, Sebastian Kusyk, Hancheng Li, Zuzanna Mianowska, Jerzy Mietelski, Agnieszka Pollo, Dominik Rybka, Jianchao Sun, Jan Swakon, Damian Wrobel, Xin Wu
{"title":"质子辐照SiPM阵列对POLAR-2的影响","authors":"Slawomir Mianowski, Nicolas De Angelis, Johannes Hulsman, Merlin Kole, Tomasz Kowalski, Sebastian Kusyk, Hancheng Li, Zuzanna Mianowska, Jerzy Mietelski, Agnieszka Pollo, Dominik Rybka, Jianchao Sun, Jan Swakon, Damian Wrobel, Xin Wu","doi":"10.1007/s10686-022-09873-6","DOIUrl":null,"url":null,"abstract":"<div><p>POLAR-2 is a space-borne polarimeter, built to investigate the polarization of Gamma-Ray Bursts and help elucidate their mechanisms. The instrument is targeted for launch in 2024 or 2025 aboard the China Space Station and is being developed by a collaboration between institutes from Switzerland, Germany, Poland and China. The instrument will orbit at altitudes between 340km and 450km with an inclination of <span>\\({42}{^{\\circ }}\\)</span> and will be subjected to background radiation from cosmic rays and solar events. It is therefore pertinent to better understand the performance of sensitive devices under space-like conditions. In this paper we focus on the radiation damage of the silicon photomultiplier arrays S13361-6075NE-04 and S14161-6050HS-04 from Hamamatsu. The S13361 are irradiated with 58MeV protons at several doses up to 4.96Gy, whereas the newer series S14161 are irradiated at doses of 0.254Gy and 2.31Gy. Their respective performance degradation due to radiation damage are discussed. The equivalent exposure time in space for silicon photomultipliers inside POLAR-2 with a dose of 4.96Gy is 62.9years (or 1.78years when disregarding the shielding from the instrument). Primary characteristics of the I-V curves are an increase in the dark current and dark counts, mostly through cross-talk events. Annealing processes at <span>\\({25}{^{\\circ }C}\\)</span> were observed but not studied in further detail. Biasing channels while being irradiated have not resulted in any significant impact. Activation analyses showed a dominant contribution of <span>\\(\\beta ^{+}\\)</span> particles around 511 keV. These resulted primarily from copper and carbon, mostly with decay times shorter than the orbital period.</p></div>","PeriodicalId":551,"journal":{"name":"Experimental Astronomy","volume":"55 2","pages":"343 - 371"},"PeriodicalIF":2.7000,"publicationDate":"2022-10-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s10686-022-09873-6.pdf","citationCount":"5","resultStr":"{\"title\":\"Proton irradiation of SiPM arrays for POLAR-2\",\"authors\":\"Slawomir Mianowski, Nicolas De Angelis, Johannes Hulsman, Merlin Kole, Tomasz Kowalski, Sebastian Kusyk, Hancheng Li, Zuzanna Mianowska, Jerzy Mietelski, Agnieszka Pollo, Dominik Rybka, Jianchao Sun, Jan Swakon, Damian Wrobel, Xin Wu\",\"doi\":\"10.1007/s10686-022-09873-6\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>POLAR-2 is a space-borne polarimeter, built to investigate the polarization of Gamma-Ray Bursts and help elucidate their mechanisms. The instrument is targeted for launch in 2024 or 2025 aboard the China Space Station and is being developed by a collaboration between institutes from Switzerland, Germany, Poland and China. The instrument will orbit at altitudes between 340km and 450km with an inclination of <span>\\\\({42}{^{\\\\circ }}\\\\)</span> and will be subjected to background radiation from cosmic rays and solar events. It is therefore pertinent to better understand the performance of sensitive devices under space-like conditions. In this paper we focus on the radiation damage of the silicon photomultiplier arrays S13361-6075NE-04 and S14161-6050HS-04 from Hamamatsu. The S13361 are irradiated with 58MeV protons at several doses up to 4.96Gy, whereas the newer series S14161 are irradiated at doses of 0.254Gy and 2.31Gy. Their respective performance degradation due to radiation damage are discussed. The equivalent exposure time in space for silicon photomultipliers inside POLAR-2 with a dose of 4.96Gy is 62.9years (or 1.78years when disregarding the shielding from the instrument). Primary characteristics of the I-V curves are an increase in the dark current and dark counts, mostly through cross-talk events. Annealing processes at <span>\\\\({25}{^{\\\\circ }C}\\\\)</span> were observed but not studied in further detail. Biasing channels while being irradiated have not resulted in any significant impact. Activation analyses showed a dominant contribution of <span>\\\\(\\\\beta ^{+}\\\\)</span> particles around 511 keV. 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POLAR-2 is a space-borne polarimeter, built to investigate the polarization of Gamma-Ray Bursts and help elucidate their mechanisms. The instrument is targeted for launch in 2024 or 2025 aboard the China Space Station and is being developed by a collaboration between institutes from Switzerland, Germany, Poland and China. The instrument will orbit at altitudes between 340km and 450km with an inclination of \({42}{^{\circ }}\) and will be subjected to background radiation from cosmic rays and solar events. It is therefore pertinent to better understand the performance of sensitive devices under space-like conditions. In this paper we focus on the radiation damage of the silicon photomultiplier arrays S13361-6075NE-04 and S14161-6050HS-04 from Hamamatsu. The S13361 are irradiated with 58MeV protons at several doses up to 4.96Gy, whereas the newer series S14161 are irradiated at doses of 0.254Gy and 2.31Gy. Their respective performance degradation due to radiation damage are discussed. The equivalent exposure time in space for silicon photomultipliers inside POLAR-2 with a dose of 4.96Gy is 62.9years (or 1.78years when disregarding the shielding from the instrument). Primary characteristics of the I-V curves are an increase in the dark current and dark counts, mostly through cross-talk events. Annealing processes at \({25}{^{\circ }C}\) were observed but not studied in further detail. Biasing channels while being irradiated have not resulted in any significant impact. Activation analyses showed a dominant contribution of \(\beta ^{+}\) particles around 511 keV. These resulted primarily from copper and carbon, mostly with decay times shorter than the orbital period.
期刊介绍:
Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments.
Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields.
Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.