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	Compact optical image amplifier pumped by a sub-nanosecond Nd:YAG microlaser 期刊论文 OAI收割 APPLIED OPTICS, 2018, 卷号: 57, 期号: 10, 页码: 2622-2626 作者: Liu, Lei; Wang, Hongyan; Ning, Yu; Ren, Ge; Yang, Yi \| 收藏 \| 浏览/下载：68/0 \| 提交时间：2019/08/23 Geometrical optics Image intensifiers (solid state) Noise figure Optical frequency conversion Phase matching Signal to noise ratio Yttrium aluminum garnet
	On the benefit of aberration-corrected HAADF-STEM for strain determination and its application to tailoring ferroelectric domain patterns 期刊论文 OAI收割 ULTRAMICROSCOPY, 2016, 卷号: 160, 页码: 57-63 Tang, Y. L.; Zhu, Y. L.; Man, X. L. 收藏 \| 浏览/下载：47/0 \| 提交时间：2016/04/21 Aberration-corrected scanning transmission electron microscopy High angle annular dark field (HAADF) Strain determination Geometrical phase analysis (GPA) Ferroelectric domain structure PbTiO3 films
	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：40/0 \| 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.
	Statistical theory for hydrogen bonding fluid system of A(a)D(d) type (I): The geometrical phase transition 期刊论文 OAI收割 Science in China Series B-Chemistry, 2006, 卷号: 49, 期号: 6, 页码: 499-506 H. J. Wang; X. Z. Hong; F. Gu; X. W. Ba 收藏 \| 浏览/下载：23/0 \| 提交时间：2012/04/14 hydrogen bonding fluid equilibrium free energy geometrical phase transition equation-of-state thermoreversible gelation liquid water computer-simulations dynamics networks polymers models
	Analyses on the geometrical structure of magnetic field in the current sheet based on cluster measurements 期刊论文 OAI收割 Journal of Geophysical Research-Space Physics, 2003, 卷号: 108, 期号: A5, 页码: 1168 Shen, C.; Li, X.; Dunlop, M.; Liu, Z. X.; Balogh, A.; Baker, D. N.; Hapgood, M.; Wang, X. 收藏 \| 浏览/下载：31/0 \| 提交时间：2014/04/30 geometrical structure of magnetosphere curvature of magnetic field lines current sheet neutral sheet flapping of neutral sheet substorm moderately disturbed conditions 3 spacecraft observations substorm growth-phase thin current sheets earth plasma sheet tail current sheet geomagnetic tail tearing instability magnetotail motion