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	基于衬底集成空心波导的气体检测性能研究期刊论文 OAI收割量子电子学报, 2023, 卷号: 40 作者: 黄文彪 \| 收藏 \| 浏览/下载：7/0 \| 提交时间：2024/11/20 waveguide optics Fourier transform infrared spectrometer substrate-integrated hollow waveguide gas detection geometric parameter 波导光学傅里叶变换红外光谱衬底集成空心波导气体检测几何参数
	Study on Laser Parameter Measurement System Based on Cone-Arranged Fibers and CCD Camera 期刊论文 OAI收割 SENSORS, 2022, 卷号: 22 作者: Luo, Jie; Qin, Laian; Hou, Zaihong; Zhang, Silong; Zhu, Wenyue \| 收藏 \| 浏览/下载：28/0 \| 提交时间：2022/12/23 laser parameter array fibers CCD camera integrated optics PIB
	CEPC cost model study and circumference optimization 期刊论文 OAI收割 Journal of Instrumentation, 2022, 卷号: 17, 期号: 10, 页码: P10018 作者: Wang, Dou; Gao, Jie; Ruan, Manqi; Li, Yuhui; Xu, Haocheng \| 收藏 \| 浏览/下载：11/0 \| 提交时间：2023/11/10 Accelerator modelling and simulations (multi-particle dynamics, single-particle dynamics) Beam dynamics Beam Optics CEPC cost performance parameter choice luminosity scan beam-beam limit circumference optimization activity report top: particle source Higgs-factory Z0-factory CEPC costs numerical calculations
	Atmospheric Optical Turbulence Characteristics over the Ocean Relevant to Astronomy and Atmospheric Physics 期刊论文 OAI收割 APPLIED SCIENCES-BASEL, 2021, 卷号: 11 作者: Xu, Manman; Shao, Shiyong; Weng, Ningquan; Zhou, Liangping; Liu, Qing \| 收藏 \| 浏览/下载：49/0 \| 提交时间：2022/01/10 optical turbulence astroclimatic parameter atmospheric physics ocean and atmospheric optics
	Two-axis gimbal platform controller design in finite time application occasions LMI approach 期刊论文 OAI收割 Optik, 2018, 卷号: 158, 页码: 831-841 作者: Chen, Y.; Chu, H. R.; Sun, T. T.; Guo, L. H.; Zhang, F. \| 收藏 \| 浏览/下载：13/0 \| 提交时间：2019/09/17 Two-axis gimbal platform Linear parameter varying state equation Finite-time boundedness LMI fuzzy controller stabilization system stability Optics
	MIA analysis of FPGA BPMs and beam optics at APS 期刊论文 OAI收割 Chinese Physics C, 2012, 期号: 11, 页码: 1120-1125 作者: Ji DH(季大恒); Wang CX(王春喜); Qin Q(秦庆) 收藏 \| 浏览/下载：27/0 \| 提交时间：2015/12/14 MIA PCA SVD FPGA BPM optics parameter lattice fitting
	Estimating leaf area index by inversion of reflectance model for semiarid natural grasslands 期刊论文 iSwitch采集 Science in china series d-earth sciences, 2009, 卷号: 52, 期号: 1, 页码: 66-84 作者: Zhang Na; Zhao YingShi 收藏 \| 浏览/下载：31/0 \| 提交时间：2019/05/10 Leaf area index Plant crown shape Geometrical similarity parameter Reflectance model Radiative transfer Geometric optics Inversion Semiarid natural grassland
	Research on the support structure of the primary mirror of large-aperture telescope (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 Yang W.; Jingxu Z. 收藏 \| 浏览/下载：28/0 \| 提交时间：2013/03/25 Large-aperture telescope can be used in surveying battlefield researching landform searching object real-time monitoring imaging detecting and identifying spatial targets and so on. A large-aperture telescope for achieving high resolution power is designed to monitor spatial target and image in real time. Real-time monitoring plays an important role in military conflicts. The orbit parameter of object quantity geometrical shape parameter and so on can be obtained by detect spatial target. With the development of optical technology people require larger aperture in optics-electronic (OE) system. By increasing optical aperture the ability of collecting light and resolution power in the system can be enhanced. But the support structure of the primary mirror of large-aperture telescope will be a very difficult problem. With the increase of primary mirror aperture the weight of the primary mirror will become larger than before. The root mean square (rms) of the primary mirror is affected by many factors such as deadweight deformation of heat environment and so on. Due to the primary mirror of telescope is an important component of telescope system. By reducing the weight of primary mirror precision of the system is ensured. During the designing phase one can consider the supporting project of the primary mirror synthetically and analyze it roundly according to technical requirement of optical system and the effect factors. The final structural design can be reasonable. In an astronomical telescope the surface of reflector is an important part for collecting dark radiation of celestial bodies. Its surface shape will have an effect on collecting efficiency of telescope radiant energy directly. So the rms must be very high. Optical system of large aperture small wavelength and small focus can receive maximal light intensity. For ground-based optical astronomical telescope the design proposed in the paper can satisfy the requirement of the possible minimum atmosphere seeing at astronomical observatory site and exert the use efficiency of the telescope adequately. So the accuracy of the traditional surface of reflector can assure that 90% of all the light energy can be focused on within the angle diameter range of the minimum atmosphere seeing then 100% of light energy should be focused on the angle diameter range of minimum atmosphere seeing. Because the rms of mirror is very high precise surface machining and accurate the support of mirror are very important tasks during designing and manufacturing the telescope. In the paper various support techniques of a large-aperture telescope primary mirror are discussed and a 3.5 meter telescope system at the Starfire Optical Range (SOR) overviewed simply which was operated by the Directed Energy Directorate of the Air Force Research Laboratory Kirtland AFB NM USA from the ground-based O-E system for the observations of spatial target. We also analyze Theoretical elastic deformation of the Steward Observatory 2.3 meter mirror is analyzed.
	Research of automatic test technology of parameters used in a dual-CCD TV measure-system (EI CONFERENCE) 会议论文 OAI收割 2nd International Symposium on Advanced Optical Manufacturing and Testing Technologies: Optical Test and Measurement Technology and Equipment, November 2, 2005 - November 5, 2005, Zian, China 作者: Wang L.; Li Y.; Li Y.; Li Y.; Li Y. 收藏 \| 浏览/下载：22/0 \| 提交时间：2013/03/25 This paper describes a kind of automatic test technology of the parameters used in a dual-CCD TV measure-system (TV -MS) .The TV -MS is the ground control equipment of the anti-tank missile and integrates the technologies of optical machine and electronics. It is important and key component. The main technical parameters of the TV -MS are field of view zero point precision sensitivity anti-jamming ability zooming time and focus time etc. To insure the TV -MS satisfying the tactical and technical requirements and discover fault and reason a fast and accurate equipment satisfying the test technical parameters of the TV -MS is urgently needed in manufacture and service. Firstly the parameter test system converted optical signal to electronic signal implemented automatic control of the invariant illumination of parallel pipeline output. Secondly data and command delivering displaying or printing are realized by using 80C196KB. The experiment result shows that the approach of automatic testing of the Parameters used in a dual-CCD TV -MS is successful and it can be used for all tests of the functions and parameters of the TV -MS. The main innovations are to realize the fast veracious measure of technical parameters of the dual-CCD TV-MS and integrate the technologies of optics machineries and electronics. An advanced means is provided to judge the technical states find malfunctions and discover the reasons in producing and maintaining process. The equipment suited for anti-tank missile systems is given.