
浏览全部资源
扫码关注微信
1.哈尔滨理工大学 理学院 黑龙江省量子调控重点实验室,黑龙江 哈尔滨 150080
2.中国科学院 高能物理研究所 中国科学院粒子天体物理重点实验室,北京 100049
[ "赵子健(1994-),男,黑龙江哈尔滨人,硕士研究生,2016年于黑龙江大学获得学士学位,主要研究方向为X射线成像。E-mail:zhaozijian@ihep.ac.cn" ]
王于仨(1982-),男,安徽人,副研究员,主要研究方向为X射线标定。E-mail:wangyusa@ihep.ac.cn WANG Yu-sa, E-mail: wangyusa@ihep.ac.cn
收稿日期:2019-06-27,
录用日期:2019-7-15,
纸质出版日期:2019-11-15
移动端阅览
赵子健, 王于仨, 张留洋, 等. Wolter-I型聚焦镜X射线光学实验与仿真[J]. 光学 精密工程, 2019,27(11):2330-2336.
Zi-jian ZHAO, Yu-sa WANG, Liu-yang ZHANG, et al. Experiments and simulation of X-ray optical Wolter-I focusing mirror[J]. Optics and precision engineering, 2019, 27(11): 2330-2336.
赵子健, 王于仨, 张留洋, 等. Wolter-I型聚焦镜X射线光学实验与仿真[J]. 光学 精密工程, 2019,27(11):2330-2336. DOI: 10.3788/OPE.20192711.2330.
Zi-jian ZHAO, Yu-sa WANG, Liu-yang ZHANG, et al. Experiments and simulation of X-ray optical Wolter-I focusing mirror[J]. Optics and precision engineering, 2019, 27(11): 2330-2336. DOI: 10.3788/OPE.20192711.2330.
为了深入研究Wolter-I型X射线聚焦镜片的光学性能,掌握聚焦镜的对准和测试方法,研究单层Wolter-I型X射线聚焦镜片性能。在中国科学院高能物理研究所(IHEP)百米真空X射线标定装置中对单层聚焦镜镜片的离焦、聚焦和离轴工况进行了实验测试。分析了焦距、焦斑分布、角分辨(50%能量所占区域HEW为17″和90%能量所占区域W90为44″)等光学性能参数。将得到的结果与德国马克斯普朗克地外物理研究所(MPE)PANTER X射线标定装置的实验数据对比,性能参数基本相同,得到的W90甚至优于MPE。实验结果验证了仿真计算结果,为进一步开展像质研究提供了依据。通过实验掌握了聚焦镜的对准和测试方法,未来该方法在X射线天文卫星载荷标定测试中将发挥巨大作用。
In order to investigate the optical performance of the Wolter-I X-ray mirror shell and to grasp the focusing and testing methods of focusing mirror
the performance of single-layer Wolter-I X-ray focusing mirror was studied. The defocusing
focusing
and off-axis conditions of single-layer focusing lens were experimentally tested in the 100-m vacuum X-ray calibration facility at the Institute of High Energy Physics
Chinese Academy of Sciences. Optical performance parameters such as focal length
focal spot distribution
angular resolution (half energy area is 17″HEW on-axis and 90% energy area is 44″W90 on-axis) were analyzed and calculated. Compared with the data of MPE
the performance parameters are basically the same
and the W90 is better than that of MPE. The experimental results agreed with the simulation results
which provides a basis for further research on image quality. Through experiments
the alignment and testing methods of focusing mirrors are mastered
which will play an important role in the load calibration testing of X-ray astronomical satellites in the future.
RAIMONDI L, SPIGA D. Point spread function of real Wolter-I X-ray mirrors: computation by means of the Huygens-Fresnel principle[J]. SPIE, 2011, 8147:81470Z-1-81470Z-13.
袁为民, 张臣, 陈勇, 等.爱因斯坦探针:探索变幻多姿的X射线宇宙[J].中国科学:物理学力学天文学, 2018, 48: 039502-1-039502-21.
YUAN W M, ZHANG C, CHEN Y, et al .. Einstein probe: exploring the ever-changing X-ray universe (in Chinese)[J]. Sci Sin-Phys Mech Astron, 2018, 48:039502-1-039502-21. (in Chinese)
YUAN W, ZHANG CH, LING ZH X, et al .. Einstein Probe: a lobster-eye telescope for monitoring the x-ray sky[J]. SPIE, 2018, 10699:1069925-1-1069925-9.
ZHANG S N, SANTANGELO A, FEROCI M, et al .. "eXTP: Enhanced X-ray timing and polarization mission"[J]. Sci. China-Phys Mech Astron, 2017, 60:1-25.
HERNANZ M, BRANDT S, FEROCI M, et al .. The wide field monitor onboard the eXTP mission[J]. SPIE , 2018, 10699:1069948-1-1069948-16.
清华天体物理中心低温探测器实验室[EB/OL]. http://hubs.phys.tsinghua.edu.cn/ http://hubs.phys.tsinghua.edu.cn/ , 2019, Copyright ® 2018-2019 HUBS Mission.
Low-temperature detection laboratory of Tsinghua Celestial Physical Center. Einstein probe: exploring the ever-changing X-ray universe[EB/OL]. http://hubs.phys.tsinghua.edu.cn/ http://hubs.phys.tsinghua.edu.cn/ , 2019, Copyright ® 2018-2019 HUBS Mission. (in Chinese)
PREDEHL P, ANDRITSCHKE R, BECKER W, et al ..eROSITA[J]. SPIE , 2011, 8145:81450D-1-81450D-10.
FREYBERG M, BUDAU B, BURKERT W, et al .. Potential of the PANTER x-ray test facility for calibration of instrumentation for XEUS[J]. SPIE, 2006, 6266:62663H-1-62663H-9.
MENZ B, BRÄUNINGER H, BURWITZ V, et al .. Studying ATHENA optics with divergent and collimated x-ray beams[J]. SPIE, 2017, 9144:91445J-1-91445J-8.
VERNANI D, BORGHI G, CALEGARI G, et al .. Performance of a mirror shell replicated from a new flight quality mandrel for eROSITA mission[J]. SPIE, 2011, 8147:814707-1-814707-9.
The center for X-ray optics[DB/OL]. http://henke.lbl.gov/optical_constants/layer2.html http://henke.lbl.gov/optical_constants/layer2.html , 2019, Copyright ® 2010 The Center for X-Ray Optics.
BURWITZ V, PREDEHL P, FRIEDRICH P, et al .. The calibration and testing of the eROSITA X-ray mirror assemblies[J]. SPIE, 2014, 9144:91441X-1-91441X-6.
BURWITZ V, WILINGALE R, PELLILCIARI C, et al .. Testing and calibrating the ATHENA optics at PANTER[J]. SPIE, 2017, 10399:103990OO-1-103990OO-7.
陆波, 王于仨, 杨彦佶, 等.基于CCD和CsI闪烁体的硬X射线成像[J].光学 精密工程, 2017, 25(11): 2865-2871.
LU B, WANG Y S, YANG Y J, et al.. Hard X-ray imaging based on CCD and Csl scintillator[J]. Opt. Precision Eng. , 2017, 25(11): 2865-2871. (in Chinese)
FRIEDRICH P, BRÄUNINGER H, BUDAU B, et al .. Development and testing of the eROSITA mirror modules[J]. SPIE, 2012, 8443:84431S-1-84431S-8.
0
浏览量
164
下载量
7
CSCD
关联资源
相关文章
相关作者
相关机构
京公网安备11010802024621