基于多元约束的小型软X射线偏振望远镜光学设计及优化

张玲; 沈正祥; 刘娜; 余俊; 王占山

doi:10.3788/IRLA201746.0718002

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

基于多元约束的小型软X射线偏振望远镜光学设计及优化

张玲, 沈正祥, 刘娜, 余俊, 王占山

文章导航 > 红外与激光工程 > 2017 > 46(7): 718002-0718002(7)

张玲, 沈正祥, 刘娜, 余俊, 王占山. 基于多元约束的小型软X射线偏振望远镜光学设计及优化[J]. 红外与激光工程, 2017, 46(7): 718002-0718002(7). doi: 10.3788/IRLA201746.0718002

引用本文:

Zhang Ling, Shen Zhengxiang, Liu Na, Yu Jun, Wang Zhanshan. Optical design and optimization of the small-scale soft X-ray polarization telescope based on multi-constraints[J]. Infrared and Laser Engineering, 2017, 46(7): 718002-0718002(7). doi: 10.3788/IRLA201746.0718002

Citation:

Zhang Ling, Shen Zhengxiang, Liu Na, Yu Jun, Wang Zhanshan. Optical design and optimization of the small-scale soft X-ray polarization telescope based on multi-constraints[J]. Infrared and Laser Engineering, 2017, 46(7): 718002-0718002(7). doi: 10.3788/IRLA201746.0718002

基于多元约束的小型软X射线偏振望远镜光学设计及优化

doi: 10.3788/IRLA201746.0718002

张玲^1,2,
沈正祥^1,2,
刘娜^1,2,
余俊^1,2,
王占山^1,2

1.
同济大学先进微结构材料教育部重点实验室,上海 200092;
2.
同济大学物理科学与工程学院精密光学工程技术研究所,上海 200092

基金项目:

国家自然科学基金（11105099，10978002）;科技部国家重大科学仪器设备开发专项（2012YQ04016403）

详细信息

作者简介:
张玲(1992-),女,硕士生,主要从事X射线光学系统设计方面的研究。Email:1334099@tongji.edu.cn

中图分类号: O434.12

Optical design and optimization of the small-scale soft X-ray polarization telescope based on multi-constraints

1.
Key Laboratory of Advanced Micro-Structure Materials,Ministry of Education,Tongji University,Shanghai 200092,China;
2.
Institute of Precision Optical Engineering,School of Physics Science and Engineering,Tongji University,Shanghai 200092,China

摘要: 作为揭示物质在强磁场、强引力场中的行为方式以及天体辐射偏振产生原因的重要手段，X射线偏振探测在近40年来一直是高能天体物理的研究热点。小型软X射线天文偏振探测望远镜采用抛物面聚焦方式将X射线会聚至探测器处，通过在反射镜表面镀制多层膜实现高反射率和能量分辨。文中对小型天文偏振望远镜抛物面的两种空间布局方式，即中心环绕旋转式镜面布局和交叉对称式镜面布局进行了理论分析，构建了综合集光面积和制作难度的优化模型，基于多元约束方式进行了参数优化。结果显示，在系统口径受限、探测器有一定尺寸的实际应用环境中，参数优化后的交叉对称式镜面布局方案较常规中心环绕式设计更有优势，既能获得较大的集光面积，又能兼顾镜面加工的可行性。
- X 射线偏振 /
- 望远镜 /
- 光学设计 /
- 多元约束 /
- 优化
Abstract: The probe of the X-ray polarization in high-energy astrophysics has been a research focus over the past 40 years, and it has been an efficient way to reveal matters' behaviors under circumstances of extreme magnetic and gravitational fields, and to understand the causation of polarization. The small-scale soft X-ray polarization telescope usually focus soft X-ray into the detection zone, and the surface type of the telescope is paraboloid. The mirror of the telescope is deposed with multilayer, it can reflect soft X-ray with a rather high reflectivity and a high energy resolution, which satisfies the Bragg condition. Here, two kinds of design configurations for a soft X-ray polarimetry mission based on paraboloidal surface shape were presented. Some calculations and analyses were done under the limitation of a specific size of the whole system. The relation was summarized between collected area, the complexity of the fabrication, and other practical application factors. The result of the optimization demonstrates that the optimized choice for the design can guarantee the practical utilization in reality.
- X-ray polarimetry /
- telescope /
- optical design /
- multi-constraints /
- optimization

[1]	Chen Jie, Liu Longhua, Liu Gang, et al. X-ray imaging Fresnel zone plates and fabrication[J]. Optics Precision Engineering, 2007, 15(12):1894-1899. (in Chinese)
[2]	Bellazzini R, Baldini L, Costa E, et al. X-ray polarimetry:a new window on the high energy sky[J]. Nuclear Instruments Methods in Physics Research, 2010, 623(2):766-770.
[3]	Silver E H, Ziock K, Weisskopf M C, et al. Bragg crystal polarimeters[J]. Optical Engineering, 1990, 29(7):759-766.
[4]	Lu Fangjun, Zhang Shuangnan, Dong Yongwei. The X-ray timing and polarization satellite[C]//National Space Exploration Seminar, 2012.
[5]	Allured R, Fernndez-Perea M, Soufli R, et al. A soft X-ray beam-splitting multilayer optic for the NASA GEMS Bragg Reflection Polarimeter[J]. Experimental Astronomy, 2012, 36(1-2):371-388.
[6]	Allured R, Fernndez-Perea M, Soufli R, et al. XIPE:the X-ray imaging polarimetry explorer[J]. Experimental Astronomy, 2013, 36(3):1-45.
[7]	She R, Feng H, Muleri F, et al. LAMP:a micro-satellite based soft X-ray polarimeter for astrophysics[C]//SPIE, 2015, 9601:96010-1-14.
[8]	Li Jia, Zhu Jie, Zhang Zhong, et al. Effect of Si barrier layers on the thermal stability of Al(1 wt.%Si)/Zr multilayers designed as EUV mirrors[J]. Infrared and Laser Engineering, 2015, 44(4):1335-1342. (in Chinese)
[9]	Li Yanan, Sun Xiaobing, Mao Yongna, et al. Spectral polarization characteristic of space target[J]. Infrared and Laser Engineering, 2012, 41(1):205-210. (in Chinese)
[10]	Marshall H L, Murray S S, Schnopper H W, et al. Realistic inexpensive soft X-ray polarimeter and the potential scientific return[C]//SPIE, 2003, 4843:360-371.
[11]	Yang Haoyu, Tian Ailing, Liu Bingcai. Sub-aperture stitching interferometry for large parabolic mirror[J]. Infrared and Laser Engineering, 2014, 43(4):1296-1300. (in Chinese)
[12]	Fu Yingding, Cheng Yuxiao, Tang Huiying. Optimization Theory Method[M]. Beijing:National Defense Industry Press, 2008:208-211. (in Chinese)
[13]	Shi Tu, Yang Yongying, Zhang Lei, et al. Surface testing methods of aspheric optical elements[J]. Chinese Optics, 2014, 7(1):26-46. (in Chinese)

[1]	宋晓莉, 孙何敏, 汪达兴, 张驰. 大型望远镜拼接弧线永磁电机电流谐波抑制 . 红外与激光工程, 2021, 50(S2): 20200393-1-20200393-8. doi: 10.3788/IRLA20200393
[2]	刘奉昌, 李威, 赵伟国, 王克军, 赵海波, 林冠宇. 临近空间望远镜次镜优化设计 . 红外与激光工程, 2021, 50(2): 20200178-1-20200178-10. doi: 10.3788/IRLA20200178
[3]	尹骁, 李英超, 史浩东, 江伦, 王超, 刘壮, 李冠霖. 用于物证搜寻的大视场变焦偏振成像光学系统设计 . 红外与激光工程, 2019, 48(4): 418006-0418006(8). doi: 10.3788/IRLA201948.0418006
[4]	穆竺, 王加科, 吴从均, 颜昌翔, 刘智颖. 偏振光谱识别光学系统的复原方法与设计 . 红外与激光工程, 2019, 48(5): 518004-0518004(8). doi: 10.3788/IRLA201948.0518004
[5]	李晓静, 郑子云, 史戈平, 高永亮. 制备光学金刚石膜的微波谐振腔设计及优化 . 红外与激光工程, 2019, 48(S2): 156-163. doi: 10.3788/IRLA201948.S216001
[6]	姚艳霞, 袁群, 陈露, 窦沂蒙, 殷慧敏, 高志山. 结合面型和视场优化策略的自由曲面设计方法 . 红外与激光工程, 2018, 47(10): 1018001-1018001(8). doi: 10.3788/IRLA201847.1018001
[7]	李钰鹏, 王智, 沙巍, 吴清文, 赵亚. 空间引力波望远镜主镜组件的结构设计 . 红外与激光工程, 2018, 47(8): 818004-0818004(7). doi: 10.3788/IRLA201847.0818004
[8]	穆永吉, 万渊, 刘继桥, 侯霞, 陈卫标. 星载激光雷达望远镜主镜光机分析与优化 . 红外与激光工程, 2018, 47(7): 718002-0718002(7). doi: 10.3788/IRLA201847.0718002
[9]	黄绪杰, 靳阳明, 潘俏, 朱嘉诚, 沈为民. 多角度偏振成像光谱仪的光学设计 . 红外与激光工程, 2017, 46(11): 1118002-1118002(7). doi: 10.3788/IRLA201746.1118002
[10]	罗小贤, 赵柏秦, 纪亚飞, 庞艺. 椭圆高斯分布半导体激光器泵浦被动调Q激光器的优化 . 红外与激光工程, 2017, 46(3): 305003-0305003(7). doi: 10.3788/IRLA201746.0305003
[11]	张伟, 张合, 张祥金. 小型大瞬时视场光学探测系统优化设计 . 红外与激光工程, 2016, 45(5): 518002-0518002(6). doi: 10.3788/IRLA201645.0518002
[12]	孟庆宇, 王维, 纪振华, 董吉洪, 李威, 王海萍. 主三镜一体化离轴三反光学系统设计 . 红外与激光工程, 2015, 44(2): 578-582.
[13]	刘洋, 方勇华, 李大成, 李扬裕. 中红外平面光栅光谱仪系统光学设计与优化 . 红外与激光工程, 2015, 44(2): 413-418.
[14]	孙雯, 胡建军, 赵知诚, 陈新华, 韩琳, 沈为民. 新型两镜折反式平场消像散望远物镜光学设计 . 红外与激光工程, 2015, 44(12): 3667-3672.
[15]	郝惠敏, 张勇, 权龙. 三电极碳纳米管传感器的极间距优化 . 红外与激光工程, 2015, 44(10): 3061-3065.
[16]	潘年, 马文礼, 黄金龙. 地基望远镜风载数值分析 . 红外与激光工程, 2015, 44(1): 134-140.
[17]	刘祥意, 张景旭, 陈宇东, 吴小霞, 李剑锋, 郝亮. 大口径主镜支撑液压缸用弹性膜片优化设计 . 红外与激光工程, 2015, 44(1): 188-194.
[18]	李冰, 赵跃进, 张超, 郭小虎, 张镜水, 孔令琴. 非成像式激光告警系统的光学设计及优化 . 红外与激光工程, 2014, 43(5): 1511-1516.
[19]	武汉, 朱向冰, 朱骞, 陈春, 王程. 数字微镜元件式自适应前照灯光学设计 . 红外与激光工程, 2013, 42(4): 955-959.
[20]	苏燕芹, 张景旭, 陈宝刚, 杨飞, 赵宏超. TMT三镜系统Rotator组件轴承设 . 红外与激光工程, 2013, 42(12): 3289-3294.

点击查看大图

计量

文章访问数: 310
HTML全文浏览量: 47
PDF下载量: 57
被引次数: 0

基于多元约束的小型软X射线偏振望远镜光学设计及优化

doi: 10.3788/IRLA201746.0718002

1. 同济大学先进微结构材料教育部重点实验室,上海 200092;

2. 同济大学物理科学与工程学院精密光学工程技术研究所,上海 200092

作者简介:
张玲(1992-),女,硕士生,主要从事X射线光学系统设计方面的研究。Email:1334099@tongji.edu.cn

收稿日期: 2016-11-06
修回日期: 2016-12-10
刊出日期: 2017-07-25

基金项目:

国家自然科学基金（11105099，10978002）;科技部国家重大科学仪器设备开发专项（2012YQ04016403）

中图分类号: O434.12

关键词:

摘要: 作为揭示物质在强磁场、强引力场中的行为方式以及天体辐射偏振产生原因的重要手段，X射线偏振探测在近40年来一直是高能天体物理的研究热点。小型软X射线天文偏振探测望远镜采用抛物面聚焦方式将X射线会聚至探测器处，通过在反射镜表面镀制多层膜实现高反射率和能量分辨。文中对小型天文偏振望远镜抛物面的两种空间布局方式，即中心环绕旋转式镜面布局和交叉对称式镜面布局进行了理论分析，构建了综合集光面积和制作难度的优化模型，基于多元约束方式进行了参数优化。结果显示，在系统口径受限、探测器有一定尺寸的实际应用环境中，参数优化后的交叉对称式镜面布局方案较常规中心环绕式设计更有优势，既能获得较大的集光面积，又能兼顾镜面加工的可行性。

English Abstract

Optical design and optimization of the small-scale soft X-ray polarization telescope based on multi-constraints

1. Key Laboratory of Advanced Micro-Structure Materials,Ministry of Education,Tongji University,Shanghai 200092,China;

2. Institute of Precision Optical Engineering,School of Physics Science and Engineering,Tongji University,Shanghai 200092,China

Received Date: 2016-11-06
Rev Recd Date: 2016-12-10
Publish Date: 2017-07-25

Keywords:

Abstract: The probe of the X-ray polarization in high-energy astrophysics has been a research focus over the past 40 years, and it has been an efficient way to reveal matters' behaviors under circumstances of extreme magnetic and gravitational fields, and to understand the causation of polarization. The small-scale soft X-ray polarization telescope usually focus soft X-ray into the detection zone, and the surface type of the telescope is paraboloid. The mirror of the telescope is deposed with multilayer, it can reflect soft X-ray with a rather high reflectivity and a high energy resolution, which satisfies the Bragg condition. Here, two kinds of design configurations for a soft X-ray polarimetry mission based on paraboloidal surface shape were presented. Some calculations and analyses were done under the limitation of a specific size of the whole system. The relation was summarized between collected area, the complexity of the fabrication, and other practical application factors. The result of the optimization demonstrates that the optimized choice for the design can guarantee the practical utilization in reality.