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光谱学与光谱分析 2024年第4期44卷 1158-1164页

作者：李文凯周亮刘朝晖崔凯刘凯李治国谢梅林中国科学院西安光学精密机械研究所陕西西安710119 中国科学院大学北京100049

对高速运动的远距离空间目标而言,温度是表征其工作状态与性能的重要参数之一。准确获取目标的温度对判别其运动状态和预测其态势发展等具有重要的参考价值。目前常用的面目标或点目标的处理方法,在小目标的辐射特性测量中将不再适用,... 详细信息

对高速运动的远距离空间目标而言,温度是表征其工作状态与性能的重要参数之一。准确获取目标的温度对判别其运动状态和预测其态势发展等具有重要的参考价值。目前常用的面目标或点目标的处理方法,在小目标的辐射特性测量中将不再适用,而光谱探测增加了目标在波长维度的可分辨信息,可以准确获取目标能量随波长的分布情况,为目标温度的反演提供了可能,极具应用潜力。无狭缝光谱仪可以降低对空间目标的跟踪和稳定精度的要求,具有结构简单、帧频高和响应速度快等特点,在天文观测和航天器观测等方面具有较高的应用价值。对目标红外辐射特性测量的光谱定标模型进行了分析,确定了红外探测器像元线性响应模型中的主要参数。为了减小成像距离对测温精度的影响,提出了一种基于距离修正的目标温度反演模型,提高了测温精度,符合实际工程实践应用中的精度需求,对红外辐射光谱测温具有一定的指导意义。

关键词：辐射特性测量无狭缝光谱仪光谱定标温度反演

Birefrmgent laterally Sheared Beam Splitter - Savart polariscope

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Birefrmgent laterally Sheared Beam Splitter - Savart polaris...

2nd International Symposium on Advanced Optical Manufacturing and Testing Technologies

作者： Chunmin Zhang Baochang zhao Bin xiangli yingcai li Zhihong Peng Shool of Science xi’an Jiaotong University xi’an 710049 People’s Republic of China xi’an institute of optics and precision mechanics Chinese Academy of Sciences xi’an 710068 People’s Republic of China

＜正＞A laterally sheared beam splitter-savart polariscope was developed based on a single birefringent component. It is a key part in a novel polarization interference imaging spectrometer. The Savart polariscope consists of two paralled plales of calcite cut at an arbitrary angle to the optics axis and can split up a ray of light incident on the surface into an ordinary ray and an extraordinary ray. The output rays are paralled laterally sheared. The Savart polariscope is 25×25×12mm3 in size. The lateral displacement is 1mm and transmissivity is about 90 percent in spectral range of 0.4-2.5μm A static polarization imaging spectrometer based on a Savart polariscope has advantage of ultra-compact size, wide field of view, high throughput and without any moving parts. The principle and construction of Savart polariscope arc described, and the experimental results of the interference imaging spectrum are given.

关键词： Birefringent crystal Savart polariscope Polarization interference imaging spectrometer

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感应读出延时线阳极光子计数探测器研究

光谱学与光谱分析 2024年第5期44卷 1291-1296页

作者：张蕊利刘永安张亚龙杨向辉刘哲苏桐赵宝升盛立志中国科学院西安光学精密机械研究所瞬态光学与光子技术国家重点实验室陕西西安710119 中国科学院大学光电学院北京100049

针对空间天文、生物荧光、光谱测量等领域对高灵敏、大面阵探测器的应用需求,研制出基于感应读出方式的延迟线阳极光子计数成像探测器。该探测器由微通道板、延时线阳极以及读出电路组成,其中延时线阳极的性能直接影响探测器的成像质量... 详细信息

针对空间天文、生物荧光、光谱测量等领域对高灵敏、大面阵探测器的应用需求,研制出基于感应读出方式的延迟线阳极光子计数成像探测器。该探测器由微通道板、延时线阳极以及读出电路组成,其中延时线阳极的性能直接影响探测器的成像质量。作为一种电荷感应读出延时线阳极,该阳极利用信号到达的时间差解码入射光子的位置,可获得高的探测灵敏度和大的成像面积,同时简化了工艺难度并提升了可靠性。设计了感应读出延时线阳极,理论分析了探测器不同设计参数及材料对感应电荷量的影响,提出了解决异层电极间感应电荷量难以平衡的方法。据此研制出了收集面积为40 mm×40 mm的位敏阳极。测试结果表明该阳极信号传输衰减小于10%,极间串扰小于3%。利用该阳极进行了光子计数成像实验,获得了优于150μm的空间分辨率,为研制可应用于天文紫外光谱测量的大面阵、高灵敏探测器提供了理论依据及实验指导。

关键词：探测器光子计数成像位敏阳极空间分辨光谱测量

星载望远镜消光材料积分散射特性测试研究(英文)

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光电工程 2024年第2期51卷 59-68页

作者：刘巍李朝辉毛振赵建科朱辉魏紫薇刘勇尹云飞中国科学院西安光学精密机械研究所陕西西安710119 中国科学院大学北京100049

在散射理论的基础上,介绍了一种星载望远镜消光材料积分散射特性测试装置,实现对星载望远镜消光材料散射特性更为全面的测量。对积分散射理论、系统构造、系统性能进行了阐述。对系统进行建模仿真分析,得到结论:消光材料的散射特性在不... 详细信息

在散射理论的基础上,介绍了一种星载望远镜消光材料积分散射特性测试装置,实现对星载望远镜消光材料散射特性更为全面的测量。对积分散射理论、系统构造、系统性能进行了阐述。对系统进行建模仿真分析,得到结论:消光材料的散射特性在不同点位和入射角下存在明显差异,系统能够测量多种条件下消光材料的散射特性,并得到消光材料全面的散射特性分布。研究结果为根据消光材料特性进行针对性设计提供了更全面、更准确的散射特性分布,为杂散光的测量与抑制、高性能光学仪器的研制与装调以及计算光学等领域的研究提供了参考。为空间引力波探测星载望远镜系统的材料选型、特性研究、杂散光分析与抑制提供了基础。

关键词：空间引力波探测星载望远镜散射分布高精度测量

CEPC Technical Design Report

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Radiation Detection Technology and Methods 2024年第1期8卷 I0003-I0016,1-1091页

作者： Waleed Abdallah Tiago Carlos Adorno de Freitas Konstantin Afanaciev Shakeel Ahmad Ijaz Ahmed xiaocong Ai Abid Aleem Wolfgang Altmannshofer Fabio Alves Weiming An Rui An Daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam Arhrib Mustafa Ashry Sha Bai Yu Bai Yang Bai Vipul Bairathi Csaba Balazs Philip Bambade Yong Ban Tripamo Bandyopadhyay Shou-Shan Bao Desmond P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Michele Bertucci xiao-Jun Bi Yuanjie Bi Tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalva Bilanishvili Deng Binglin Denis Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri Angelo Bosotti Vincent Boudry Mohammed Boukidi Igor Boyko Ivanka Bozovic Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari Vladimir Bytev Giacomo Cacciapaglia Hua Cai Wenyong Cai Wujun Cai Yijian Cai Yizhou Cai Yuchen Cai Haiying Cai Huacheng Cai Lorenzo Calibbi Junsong Cang Guofu Cao Jianshe Cao Antoine Chance Xuejun Chang Yue Chang Zhe Chang xinyuan Chang Wei Chao Auttakit Chatrabhuti Yimin Che Yuzhi Che Bin Chen Danping Chen Fuqing Chen Fusan Chen Gang Chen Guoming Chen Hua-xing Chen huirun Chen Jinhui Chen Ji-Yuan Chen Kai Chen Mali Chen Mingjun Chen Mingshui Chen Ning Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaomin Chen Shiqiang Chen Tianlu Chen Wei Chen xiang Chen xiaoyu Chen xin Chen Xun Chen Xurong Chen Ye Chen Ying Chen Yukai Chen Zelin Chen Zilin Chen Gang Chen Boping Chen Chunhui Chen Hok Chuen Cheng Huajie Cheng Shan Cheng Tongguang Cheng Yunlong Chi Pietro Chimenti Wen Han Chiu Guk Cho Ming-Chung Chu xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Crivellin Hanhua Cui xiaohao Cui zhaoyuan Cui Brunella D'Anzi ling-Yun Dai xinchen Dai Xuwen Dai Antonio De Maria Nicola De Filippis Christophe De La Taille Francesca De Mori Chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhupal Dev Tang Dewen Biagio Di Micco Ran Ding Siqin Dingl Yadong Ding Haiyi Dong Jianin AGH University of Science and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui University HefeiAnhui Applied Physics Department Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu University Institute of ScienceVaranasi Bandirma Onyedi Eylul University Bandirma Beihang University Beijing Beijing Computational Science Research Center Beijing Beijing Conveyi LTD Beijing Beijing Glass Research institute Co. LtdBeijing Beijing institute of Technology Beijing Beijing Normal University Beijing Brown University ProvidenceRI Budker institute of Nuclear Physics Novosibirsk Cadi Ayyad University Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech Cairo University Giza Center for Theory and Computation National Tsing Hua UniversityHsinchu Central China Normal University WuhanHubei Central South University ChangshaHunan Centro de Fisica Teorica de Particulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&TV Equipment Co. LtdChengduSichuan China academy of engineering physics MianyangSichuan China building materials academy Beijing China Center of Advanced Science and Technology Beijing China institute of Atomic Energy Beijing China Jiliang University HangzhouZhejiang China Nuclear Instrument CO. LTDBeijing China University of Geosciences Beijing China University of Geosciences WuhanHubei China University of Mining and Technology XuzhouJiangsu China West Normal University NanchongSichuan Chongqing University Department of PhysicsChongqing Chulalongkorn University Bangkok City University of Hong Kong Department of PhysicsHong Kong Cockcroft institute Daresbury Cornell University IthacaNY CPPM(AMU/IPhU&CNRS/INP) Marseille Dalian Minzu University DalianLiaoning Dalian University of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov Laboratory of Nuclear Problems of Joint institute for Nuclear Research(DLNP JINR) Dubna East China University Of Science And Technol

The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensive collaboration with international *** complex comprises four accelerators:a 30 GeV linac,a 1.1 GeV Damping Ring,a Booster capable of achieving energies up to 180 GeV,and a Collider operating at varying energy modes(Z,W,H,and tt).The linac and Damping Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future expansion with provisions for a potential Super Proton Proton Collider(SPPC).The CEPC primarily serves as a Higgs *** its baseline design with synchrotron radiation(SR)power of 30 MW per beam,it can achieve a luminosity of 5×10^(34)cm^(-2)s^(-1)per interaction point(IP),resulting in an integrated luminosity of 13 ab^(-1)for two IPs over a decade,producing 2.6 million Higgs *** the SR power to 50 MW per beam expands the CEPC's capability to generate 4.3 million Higgs bosons,facilitating precise measurements of Higgs coupling at sub-percent levels,exceeding the precision expected from the HL-LHC by an order of *** Technical Design Report(TDR)follows the Preliminary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),comprehensively detailing the machine's layout,performance metrics,physical design and analysis,technical systems design,R&D and prototyping efforts,and associated civil engineering ***,it includes a cost estimate and a preliminary construction timeline,establishing a framework for forthcoming engineering design phase and site selection *** is anticipated to begin around 2027-2028,pending government approval,with an estimated duration of 8 *** commencement of experiments and data collection could potentially be initiated in the mid-2030s.

关键词： initiated exceeding precise

light-controlled pulsed x-ray tube with photocathode

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Chinese Physics B 2021年第11期30卷 650-655页

作者： Hao Xuan Yong-An liu Peng-Fei Qiang Tong Su xiang-hui Yang li-Zhi Sheng Bao-Sheng zhao State Key Laboratory of Transient optics and Photonics Xi’an Institute of Optics and Precision MechanicsChinese Academy of Sciences (CAS)Xi’an 710119China University of Chinese Academy of Sciences Beijing 100049China

Unstable mechanical structure,low energy efficiency,and cooling requirements limit the application of conventional x-ray tubes based on filament as cathode in several academic *** this paper,we demonstrate a light-controlled pulsed x-ray tube using multialkali cathode as electron *** photocathode active area of the light controlled x-ray tube is 13.2 cm^(2)(41 mm in diameter),which provides high photoelectron-emitting efficiency up to 0.288 mA/lm in 460-nm LED and 2.37-mA maximum tube ***,the modulation ability from 1 kHz to 100 kHz of the x-ray tube is *** results suggest that the light-controlled pulsed x-ray tube has easy modulation and short x-ray pulse properties and is promising to be the next generation x-ray tube with wide applications in medical radiation therapy as well as the calibration for detectors and scintillators.

关键词： x-ray source photocathode x-ray modulation

The Lyman-alpha Solar Telescope (LST) for the ASO-S mission——Ⅰ. Scientific objectives and overview

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Research in Astronomy and Astrophysics 2019年第11期19卷 23-32页

作者： hui li Bo Chen li Feng Ying li Yu Huang Jing-Wei li Lei Lu Jian-Chao Xue Bei-li Ying Jie zhao Yu-Tong Yang Wei-Qun Gan Cheng Fang Ke-Fei Song Hong Wang Quan-Feng Guo ling-Ping He Bo Zhu Cheng Zhu Lei Deng Hai-Chao Bao Cai-xia Cao Zhong-Guang Yang Key Laboratory of Dark Matter and Space Astronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjing 210034China School of Astronomy and Space Science University of Science and Technology of ChinaHefei 230026China Changchun institute of optics FineMechanics and PhysicsChinese Academy of SciencesChangchun 130033China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China xi’an institute of optics and precision mechanics Chinese Academy of SciencesXi’an 710119China Innovation Academy for Microsatellites Chinese Academy of SciencesShanghai 201210China

As one of the payloads for the Advanced Space-based Solar Observatory(ASO-S)mission,the Lyman-alpha(Lyα)Solar Telescope(LST)is aimed at imaging the Sun and the inner corona up to 2.5 R⊙(mean solar radius)in both the Lyα(121.6 nm)and visible wavebands with high temporo-spatial resolution,mainly targeting solar flares,coronal mass ejections(CMEs)and filaments/*** observations allow us to trace solar eruptive phenomena from the disk center to the inner corona,to study the relationships between eruptive prominences/filaments,solar flares and CMEs,to explore the dynamical processes and evolution of solar eruptions,to diagnose solar winds,and to derive physical parameters of the solar *** is actually an instrument suite,which consists of a Solar Disk Imager(SDI),a Solar Corona Imager(SCI),a White-light Solar Telescope(WST)and two Guide Telescopes(GTs).This is the first paper in a series of LST-related *** this paper,we introduce the scientific objectives,present an overview of the LST payload and describe the planned *** detailed design and data along with potential diagnostics are described in the second(Paper II)and third(Paper III)papers,respectively,appearing in this issue.

关键词： Sun flares-Sun coronal mass ejections(CMEs)-Sun filaments,prominences-Sun corona-Sun chromosphere-Sun UV radiation

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光学复用大视场成像研究

光子学报 2020年第9期49卷 126-132页

作者：周亮刘凯刘朝晖段晶李治国中国科学院西安光学精密机械研究所西安710119

为了简化光学复用成像系统复杂度和降低对编码方式的要求,基于反射镜旋转完成通道编码,构建了结合分束镜和光学成像系统实现双通道混叠成像的实验装置.为实现混叠图像的有效解混叠,提出了利用特征点检测与匹配方法实现多幅混叠图像之间... 详细信息

为了简化光学复用成像系统复杂度和降低对编码方式的要求,基于反射镜旋转完成通道编码,构建了结合分束镜和光学成像系统实现双通道混叠成像的实验装置.为实现混叠图像的有效解混叠,提出了利用特征点检测与匹配方法实现多幅混叠图像之间平移量的自动识别,进而构建出具有亚像素精度的双通道光学复用成像系统的系统复用矩阵,并采用梯度投影稀疏重建算法完成基于多幅图像的双通道图像重建,最终实验实现了光学成像系统视场角的2倍放大.此外,对所提方法在其他场景的适应性也进行了实验验证,表明了其可在不改变焦平面探测器的情况下实现光学成像系统视场角的有效放大,大大节约了大视场光学成像系统的研制成本.

关键词：复用成像大视场通道编码复用矩阵解混叠

基于各向异性及后加速技术的百飞秒时间分辨条纹管设计

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物理学报 2023年第24期72卷 302-311页

作者：田丽萍沈令斌陈萍刘玉柱陈琳惠丹丹陈希儒赵卫薛彦华田进寿金陵科技学院网络与通信工程学院南京211169 中国科学院西安光学精密机械研究所中科院超快诊断技术重点实验室西安710119 南京信息工程大学大气科学学院南京210044

减小空间电荷效应及扫描偏转系统边缘场效应引起的时间弥散是实现百飞秒级时间分辨条纹管的关键.本文提出并设计了一种新型飞秒条纹管,结合超高加速电场、高扫描速度和后加速电场的设计,可在光电阴极4 mm×10μm的范围内实现100 fs量级... 详细信息

减小空间电荷效应及扫描偏转系统边缘场效应引起的时间弥散是实现百飞秒级时间分辨条纹管的关键.本文提出并设计了一种新型飞秒条纹管,结合超高加速电场、高扫描速度和后加速电场的设计,可在光电阴极4 mm×10μm的范围内实现100 fs量级的时间分辨率.通过优化设计加速电极结构,使光电阴极有效探测范围内的电子均可在15 kV/mm量级的强电场中加速运行,有效地抑制了电子脉冲的物理时间弥散;在阳极入口处放置窄狭缝以减小大角度光电子引起的时空弥散对性能的影响;最后在荧光屏处设置+5000 V的高电位,以缩短光电子在等位区的渡越时间,进一步减小空间电荷效应引起的时间弥散.最终,此设计方法能够将条纹管的时间分辨率提高至百飞秒量级.

关键词：各向异性聚焦技术后加速技术时间分辨率飞秒条纹管