Radiation effects on scientific complementary metal-oxide-semiconductor detectors for x-ray astronomy: II. Total ionizing dose irradiation

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI:10.1117/1.jatis.10.2.026001
Mengxi Chen, Zhixing Ling, Mingjun Liu, Qinyu Wu, Chen Zhang, Jiaqiang Liu, Zhenlong Zhang, Weimin Yuan, Shuang-Nan Zhang
{"title":"Radiation effects on scientific complementary metal-oxide-semiconductor detectors for x-ray astronomy: II. Total ionizing dose irradiation","authors":"Mengxi Chen, Zhixing Ling, Mingjun Liu, Qinyu Wu, Chen Zhang, Jiaqiang Liu, Zhenlong Zhang, Weimin Yuan, Shuang-Nan Zhang","doi":"10.1117/1.jatis.10.2.026001","DOIUrl":null,"url":null,"abstract":"Complementary metal-oxide-semiconductor (CMOS) detectors are a competitive choice for current and upcoming astronomical missions. To understand the performance variations of CMOS detectors in the space environment, we investigate the total ionizing dose effects on custom-made large-format X-ray CMOS detectors. Three CMOS detector samples were irradiated with a Co60 source with a total dose of 70 and 105 krad. We test and compare the performance of these detectors before and after irradiation. After irradiation, the dark current increases by roughly 20∼100 times, and the readout noise increases from 3 e− to 6 e−. The bias level at 50 ms integration time decreases by 13 to 18 digital number (DN) at −30°C. The energy resolution increases from ∼150 to ∼170 eV at 4.5 keV at −30°C. The conversion gain of the detectors varies for <2% after the irradiation. Furthermore, there are about 50 pixels in which bias at 50 ms has changed by more than 20 DN after the exposure to the radiation and about 30 to 140 pixels in which the readout noise has increased by over 20 e− at −30°C at 50 ms integration time. These results demonstrate that the performances of large-format CMOS detectors do not suffer significant degeneration in space environment.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":1.7000,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Astronomical Telescopes Instruments and Systems","FirstCategoryId":"5","ListUrlMain":"https://doi.org/10.1117/1.jatis.10.2.026001","RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ENGINEERING, AEROSPACE","Score":null,"Total":0}
引用次数: 0

Abstract

Complementary metal-oxide-semiconductor (CMOS) detectors are a competitive choice for current and upcoming astronomical missions. To understand the performance variations of CMOS detectors in the space environment, we investigate the total ionizing dose effects on custom-made large-format X-ray CMOS detectors. Three CMOS detector samples were irradiated with a Co60 source with a total dose of 70 and 105 krad. We test and compare the performance of these detectors before and after irradiation. After irradiation, the dark current increases by roughly 20∼100 times, and the readout noise increases from 3 e− to 6 e−. The bias level at 50 ms integration time decreases by 13 to 18 digital number (DN) at −30°C. The energy resolution increases from ∼150 to ∼170 eV at 4.5 keV at −30°C. The conversion gain of the detectors varies for <2% after the irradiation. Furthermore, there are about 50 pixels in which bias at 50 ms has changed by more than 20 DN after the exposure to the radiation and about 30 to 140 pixels in which the readout noise has increased by over 20 e− at −30°C at 50 ms integration time. These results demonstrate that the performances of large-format CMOS detectors do not suffer significant degeneration in space environment.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
用于 X 射线天文学的科学互补金属氧化物半导体探测器的辐射效应:II.总电离剂量辐照
互补金属氧化物半导体(CMOS)探测器是目前和即将进行的天文任务的一个有竞争力的选择。为了了解 CMOS 探测器在太空环境中的性能变化,我们研究了总电离剂量对定制大尺寸 X 射线 CMOS 探测器的影响。三个 CMOS 探测器样品分别接受了总剂量为 70 krad 和 105 krad 的 Co60 源辐照。我们测试并比较了这些探测器在辐照前后的性能。辐照后,暗电流大约增加了 20∼100 倍,读出噪声从 3 e- 增加到 6 e-。在-30°C 时,50 毫秒积分时间的偏置水平降低了 13 至 18 个数字(DN)。在 -30°C 温度下,4.5 keV 的能量分辨率从 150 eV 增加到 170 eV。辐照后,探测器的转换增益变化小于 2%。此外,约有 50 个像素在 50 毫秒的偏压变化超过 20 DN,约有 30 至 140 个像素在 50 毫秒的积分时间内,读出噪声在-30°C 下增加了 20 e- 以上。这些结果表明,大尺寸 CMOS 探测器的性能在空间环境中不会出现明显退化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
期刊最新文献
Design, implementation, and performance of the primary reflector for SALTUS Solar system science with the Single Aperture Large Telescope for Universe Studies space observatory Milky Way and nearby galaxy science with the SALTUS space observatory Adjustable X-ray optics: thin-film actuator measurement and figure correction performance FIREBall-2 UV balloon telescope in-flight calibration system
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1