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	Catadioptric optical system design of 15-magnitude star sensor with large entrance pupil diameter 期刊论文 OAI收割 Sensors (Switzerland), 2020, 卷号: 20, 期号: 19, 页码: 1-14 作者: Bai, Yang; Li, Jianlin; Zha, Rongwei; Wang, Ying; Lei, Guangzhi \| 收藏 \| 浏览/下载：65/0 \| 提交时间：2020/11/02 star sensor catadioptric optical system COS large entrance pupil diameter di use spot 15-magnitude
	Crystal-Defect-Dependent Gas-Sensing Mechanism of the Single ZnO Nanowire Sensors 期刊论文 OAI收割 ACS SENSORS, 2018, 卷号: 3, 期号: 11, 页码: 2385, 2393 作者: Zhou, XY; Wang, AQ; Wang, Y; Bian, LZ; Yang, ZX \| 收藏 \| 浏览/下载：65/0 \| 提交时间：2018/12/29 ZnO nanowires TIN OXIDE microphotoluminescence MICRO-PHOTOLUMINESCENCE diameter OXYGEN-CHEMISORPTION space charge layer FLOWER-LIKE crystal defects ZINC-OXIDE gas sensor ETHANOL TEMPERATURE NANOSTRUCTURES SURFACE FILMS
	Characterization of Electrical Capacitance Tomography Sensors With Different Diameter 期刊论文 OAI收割 IEEE SENSORS JOURNAL, 2014, 卷号: 14, 期号: 7, 页码: 2240-2251 作者: Ye, Jiamin; Wang, Haigang; Yang, Wuqiang 收藏 \| 浏览/下载：34/0 \| 提交时间：2015/12/17 Electrical capacitance tomography sensor diameter experimental study numerical simulation
	Effect of pinhole diameter on correction accuracy of closed-loop adaptive optics system using self-referencing interferometer wavefront sensor 期刊论文 OAI收割 ACTA PHYSICA SINICA, 2010, 卷号: 59, 期号: 11, 页码: 8280-8286 作者: Bai Fu-Zhong; Rao Chang-Hui 收藏 \| 浏览/下载：58/0 \| 提交时间：2015/09/21 adaptive optics self-referencing interferometer wavefront sensor pinhole diameter closed-loop correction
	Effect of pinhole diameter on measurement accuracy of self-referencing interferometer wavefront sensor 期刊论文 OAI收割 ACTA PHYSICA SINICA, 2010, 卷号: 59, 期号: 6, 页码: 4056-4064 作者: Bai Fu-Zhong; Rao Chang-Hui 收藏 \| 浏览/下载：41/0 \| 提交时间：2015/09/21 adaptive optics self-referencing interferometer wavefront sensor pinhole diameter intensity transmission
	Research of active supporting technology based on 400mm thin mirror (EI CONFERENCE) 会议论文 OAI收割 5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Large Mirrors and Telescopes, April 26, 2010 - April 29, 2010, Dalian, China 作者: Liu X.-Y.; Wang J.-L.; Wang J.-L.; Liu X.-Y. 收藏 \| 浏览/下载：46/0 \| 提交时间：2013/03/25 Using a spherical mirror of 400mm diameter and 12mm thickness active supporting technology of thin mirror is researched. The axial support of the mirror is composed of 12 active supports and 3 fixed supports. The force actuator which is composed of displacement actuator and force sensor is installed in the active support. The mirror surface is tested by Zygo interferometer. For calibration each actuator exerts unit force alone and the surface variation is tested and taken as the response function of the actuator. The response functions of all actuators compose the stiffness matrix. Then the stiffness matrix is used by damped least square method to determine the correction force of each active support. In order to analyze the correction capability of the active supports 14 Zernike modes of the mirror surface are generated and tested respectively and 7 modes are selected for correction. Initially the RMS error of mirror surface is 1.16 I( =0.6328nm)when all actuators exert the same force. After 5 iterations the RMS error of mirror surface is reduced to 0.13 close to the original surface quality. 2010 Copyright SPIE - The International Society for Optical Engineering.
	Design and analysis of large spaceborne light-weighted primary mirror and its support system (EI CONFERENCE) 会议论文 OAI收割 3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Large Mirrors and Telescopes, July 8, 2007 - July 12, 2007, Chengdu, China Yan Y.; Jin G.; Yang H.-B. 收藏 \| 浏览/下载：42/0 \| 提交时间：2013/03/25 With the development of the resolution of spaceborne remote sensor the diameter of the primary mirror of spaceborne telescope becomes larger and larger. The distortion of primary mirror which is influenced by the mirror material structure self-weight support system and temperature environment affects optical image quality finally. In this paper an on-axis TMA high-resolution Cassegrain optical payload with a primary mirror whose diameter is 650mm was designed and the effects of the influence factors of the distortion acts on the on-axis TMA optical system primary mirror had been analyzed by means of Finite Element Analysis. During work the technology of the primary mirror design had been summarized and general consideration of the primary mirror design technology also had been described at the same time. Considering the telescope manufacture and work station a reasonable and optimal structure of the primary mirror sub-assembly is taken finally. In the end the distortion of the primary mirror during its fabrication station and work station had been analyzed by integrated Finite Element Analysis Method. The results implicated the synthesis profile error (P-V value) for the primary mirror is less than /10 and all the indexes of the primary mirror satisfy the requirements of the optical system.