The CIS115: a CMOS sensor qualified for optical imaging in the Jovian environment (Conference Presentation)

M. Soman, E. Allanwood, D.-D. Lofthouse-Smith, A. Holland, K. Stefanov, M. Leese, P. Turner
{"title":"The CIS115: a CMOS sensor qualified for optical imaging in the Jovian environment (Conference Presentation)","authors":"M. Soman, E. Allanwood, D.-D. Lofthouse-Smith, A. Holland, K. Stefanov, M. Leese, P. Turner","doi":"10.1117/12.2309799","DOIUrl":null,"url":null,"abstract":"The European Space Agency’s (ESA’s) Jupiter Icy Moon Explorer will spend 8 years transiting to the Jovian environment after launching from French Guiana in 2022. The spacecraft’s 10 scientific instruments, including a high resolution optical imager called JANUS, will explorer the Jovian system for a mission duration of 3 years studying the icy surfaces of Ganymede, Callisto and Europa and atmosphere of Jupiter. Using the combination of a 13 slot filter wheel and a back-illuminated CMOS image sensor, the JANUS camera will perform colour mapping and imaging at wavelengths between 350 nm and 1064 nm and resolutions of up to 10 m/pixel resolution during a Ganymede orbital phase.\n\nThe CIS115 is a rolling shutter image sensor from Teledyne-e2v that has been selected for JANUS. It is back-illuminated and anti-reflection coated in order to optimise detection efficiency in its 3 MPixel imaging area. Its 4T architecture reduces the dark current in the pinned photodiode collecting area to approximately 13 pA/cm^2 at 20˚C and allows the device to be operated with correlated double sampling for a readout noise performance of 5 electrons rms. In preparation for its use in JANUS, the CIS115 has undergone a thorough qualification programme, including exposure to ionising and non-ionising radiation levels of up to 200 krad(Si) and 2x10^10 protons/cm^2 (10 MeV equivalent), and a single event effect test campaign.\n\nThe CIS115 device qualification is now complete and results from the radiation test campaigns are being used to predict the expected performance at various phases of the mission as radiation damage is accumulated in the sensor. Dark current is the primary performance characteristic that has been observed to degrade with irradiation, and predicting the device’s performance at the end of life allows the maximum operating temperature of the detector to be set and justified. Additionally, behaviour observed during the qualification testing has led to optimised readout schemes that reduce the device image lag performance across the dynamic range to below the 0.1% level.","PeriodicalId":359588,"journal":{"name":"High Energy, Optical, and Infrared Detectors for Astronomy VIII","volume":"16 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-07-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"High Energy, Optical, and Infrared Detectors for Astronomy VIII","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2309799","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1

Abstract

The European Space Agency’s (ESA’s) Jupiter Icy Moon Explorer will spend 8 years transiting to the Jovian environment after launching from French Guiana in 2022. The spacecraft’s 10 scientific instruments, including a high resolution optical imager called JANUS, will explorer the Jovian system for a mission duration of 3 years studying the icy surfaces of Ganymede, Callisto and Europa and atmosphere of Jupiter. Using the combination of a 13 slot filter wheel and a back-illuminated CMOS image sensor, the JANUS camera will perform colour mapping and imaging at wavelengths between 350 nm and 1064 nm and resolutions of up to 10 m/pixel resolution during a Ganymede orbital phase. The CIS115 is a rolling shutter image sensor from Teledyne-e2v that has been selected for JANUS. It is back-illuminated and anti-reflection coated in order to optimise detection efficiency in its 3 MPixel imaging area. Its 4T architecture reduces the dark current in the pinned photodiode collecting area to approximately 13 pA/cm^2 at 20˚C and allows the device to be operated with correlated double sampling for a readout noise performance of 5 electrons rms. In preparation for its use in JANUS, the CIS115 has undergone a thorough qualification programme, including exposure to ionising and non-ionising radiation levels of up to 200 krad(Si) and 2x10^10 protons/cm^2 (10 MeV equivalent), and a single event effect test campaign. The CIS115 device qualification is now complete and results from the radiation test campaigns are being used to predict the expected performance at various phases of the mission as radiation damage is accumulated in the sensor. Dark current is the primary performance characteristic that has been observed to degrade with irradiation, and predicting the device’s performance at the end of life allows the maximum operating temperature of the detector to be set and justified. Additionally, behaviour observed during the qualification testing has led to optimised readout schemes that reduce the device image lag performance across the dynamic range to below the 0.1% level.
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
CIS115:一种适合木星环境下光学成像的CMOS传感器(会议报告)
欧洲航天局(ESA)的木星冰月探测器将于2022年从法属圭亚那发射,将用8年的时间过渡到木星环境。该航天器的10个科学仪器,包括名为JANUS的高分辨率光学成像仪,将在为期3年的任务中探索木星系统,研究木卫三、木卫四和木卫二的冰层表面以及木星的大气层。使用13槽滤光轮和背照CMOS图像传感器的组合,JANUS相机将在Ganymede轨道阶段执行波长在350 nm到1064 nm之间的彩色映射和成像,分辨率高达10米/像素。CIS115是Teledyne-e2v的滚动快门图像传感器,已被JANUS选中。它是背照和抗反射涂层,以优化其3百万像素成像区域的检测效率。其4T架构可在20˚C时将固定光电二极管收集区的暗电流降低至约13 pA/cm^2,并允许器件以相关双采样操作,读出噪声性能为5电子rms。为了准备在JANUS中使用,CIS115经过了彻底的认证程序,包括暴露于高达200克拉(Si)和2 × 10^10质子/cm^2(10兆电子伏特当量)的电离和非电离辐射水平,以及单事件效应测试活动。CIS115装置的鉴定现在已经完成,辐射测试活动的结果正在用于预测任务各个阶段的预期性能,因为传感器中累积了辐射损伤。暗电流是观察到的主要性能特征,随着辐照而降低,预测设备在使用寿命结束时的性能可以设置和证明探测器的最高工作温度。此外,在鉴定测试期间观察到的行为导致了优化的读出方案,将设备图像延迟性能在动态范围内降低到0.1%以下。
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
自引率
0.00%
发文量
0
期刊最新文献
The impact of the brighter-fatter effect on the performance of the JWST fine guidance sensor (Erratum) Front Matter: Volume 10709 The status of the detector developments supported by the European Space Agency CCD linearity measurement by incremental binning (Conference Presentation) A megapixel class HgCdTe linear mode avalanche photo-diode array for low background astronomy (Conference Presentation)
×
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