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	A portable S-DIMM developed for preliminary measurement of seeing for Solar Site Survey: Theory and one case study 期刊论文 OAI收割 NEW ASTRONOMY, 2024, 卷号: 109 作者: Duan, Xiao-Mei; Liu Y(刘煜); Song TF(宋腾飞); Zhu, Feng-Rong \| 收藏 \| 浏览/下载：29/0 \| 提交时间：2024/05/13 Atmospheric turbulence Daytime seeing Atmospheric coherence length Astronomical site survey
	Astronomical Site Monitoring System at Lijiang Observatory 期刊论文 OAI收割 RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2020, 卷号: 20, 期号: 9, 页码: 18 作者: \| 收藏 \| 浏览/下载：42/0 \| 提交时间：2020/11/30 Astronomical Site Monitoring System Lijiang Observatory Cloud Sensor Autonomous-DIMM
	全自动野外无人值守环境监测设备实施方案研究报告 OAI收割 2018 作者: 白春海 \| 收藏 \| 浏览/下载：49/0 \| 提交时间：2019/07/10 天文选址自动采集远程控制 Astronomical site selection automatic acquisition remote control
	Status of the first Antarctic Survey Telescopes for Dome A 会议论文 OAI收割 Amsterdam, Netherlands, 2012-7-1 作者: Daxing Wang; Xiangqun Cui; Xiangyan Yuan; Xuefei Gong; Lingzhe Xu 收藏 \| 浏览/下载：59/0 \| 提交时间：2014/01/09 Astronomical site Dome A Antarctica Survey Telescope Automatic observations
	An updated astronomical timescale for the Plio-Pleistocene deposits from South China Sea and new insights into Asian monsoon evolution 期刊论文 OAI收割 QUATERNARY SCIENCE REVIEWS, 2011, 卷号: 30, 期号: 13-14, 页码: 1560-1575 作者: Ao, Hong; Dekkers, Mark J.; Qin, Li; Xiao, Guoqiao \| 收藏 \| 浏览/下载：26/0 \| 提交时间：2018/09/26 Astronomical chronology South China Sea ODP Site 1143 Asian monsoon Pliocene Pleistocene
	An updated astronomical timescale for the Plio-Pleistocene deposits from South China Sea and new insights into Asian monsoon evolution 期刊论文 OAI收割 QUATERNARY SCIENCE REVIEWS, 2011, 卷号: 30, 期号: 13-14, 页码: 1560-1575 作者: Ao, Hong; Dekkers, Mark J.; Qin, Li; Xiao, Guoqiao \| 收藏 \| 浏览/下载：17/0 \| 提交时间：2018/09/26 Astronomical chronology South China Sea ODP Site 1143 Asian monsoon Pliocene Pleistocene
	Astronomical dating of the Xiantai, Donggutuo and Maliang Paleolithic sites in the Nihewan Basin (North China) and implications for early human evolution in East Asia 期刊论文 OAI收割 PALAEOGEOGRAPHY PALAEOCLIMATOLOGY PALAEOECOLOGY, 2010, 卷号: 297, 期号: 1, 页码: 129-137 H. Ao; C.L. Cheng; M.J. Dekkers; Q.S. Liu; L. Qin; G.Q. Xiao; H. Chang 收藏 \| 浏览/下载：57/0 \| 提交时间：2011/05/04 Astronomical chronology Paleolithic site Nihewan Basin Pleistocene Human evolution
	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：32/0 \| 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.