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	Analysis and suppression of stray light in phenological network multi-spectral camera 会议论文 OAI收割 Chengdu, China, 2018-06-26 作者: Lei, Jiao; Ma, Xiaolong; Yang, Jianfeng; Xue, Bin; Lv, Juan \| 收藏 \| 浏览/下载：32/0 \| 提交时间：2019/03/22
	A novel self-deployable baffle with vanes driven by rectangular section curving tape springs 会议论文 OAI收割 Proceedings of SPIE: 7th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Optical Test and Measurement Technology and Equipment, 2014 作者: Du, Kai; Liao, Sheng; Li, Hua; Zhang, Yong 收藏 \| 浏览/下载：12/0 \| 提交时间：2016/11/23
	Study on ultra-light secondary baffle for coaxial two-mirror telescope (EI CONFERENCE) 会议论文 OAI收割 2012 9th IEEE International Conference on Mechatronics and Automation, ICMA 2012, August 5, 2012 - August 8, 2012, Chengdu, China 作者: Zhang L.; Zhang L. 收藏 \| 浏览/下载：44/0 \| 提交时间：2013/03/25 The coaxial two-mirror telescope consists of two mirrors facing each other. Classical two-mirror arrangements are Gregorian and Cassegrain. These systems are usually applied to space telescopes and often have optical baffles to prevent stray light from entering the focal plane. The optical baffles consist of concentric rings suspended between the secondary and the primary mirror. The secondary baffle for a large two-mirror optical system is designed and analyzed in this paper. According to mission of a telescope the structure should have high stiffness and high reliability and light weight. Compared with invar aluminum alloy and titanium alloy carbon fiber composite is currently the best material in terms of weight-to-strength ratio. It also has advantages of high temperature tolerance and low thermal expansion. So carbon fiber composite is chosen as material to meet requirements of the coaxial telescope. In this paper optimization method based on finite element analysis (FEA) is used for design the secondary baffle. Minimum weight of the baffle is chosen as an objective function. Thicknesses of former tube and vanes are chosen as variables. Analysis results show that the designed secondary baffle has maximum diameter of 180mm total length of 120mm and weighs 142g. And its fundamental frequency reaches 651Hz. Therefore the baffle has many advantages such as ultra-light weight high stiffness and dimensional stability etc. The optimization method and the baffle design can be helpful to other coaxial telescopes such as Cassegrain Gregorian and their subdivisions. 2012 IEEE.
	Analysis to stray radiation of infrared detecting system 会议论文 OAI收割 international symposium on photoelectronic detection and imaging 2011: advances in infrared imaging and applications, beijing, china, may 24, 2011 - may 24, 2011 NiuJin-Xing; ShiShuheng; ZhouRen-Kui 收藏 \| 浏览/下载：19/0 \| 提交时间：2012/07/09 infrared detecting system stray radiation thermal emission TracePro
	Modeling of ammonothermal growth processes of GaN crystal in large-size pressure systems 会议论文 OAI收割 2nd International Solvothermal and Hydrothermal-Association Conference (ISHA 2010), Beijing, PEOPLES R CHINA, JUL 27-29, 2010 作者: Chen QS(陈启生); Jiang YN(姜燕妮); Li W(李炜); Yan JY(颜君毅); Jiang YN(姜燕妮) 收藏 \| 浏览/下载：15/0 \| 提交时间：2012/04/01 GaN Ammonothermal growth Baffle opening Fluid flow Thermal fields
	DEM simulations on the heat conduction in a particle mixer 会议论文 OAI收割 Taiyuan, Shanxi, China, June 22, 2012 - June 24, 2012 作者: Xu, Yupeng; Cui, Lijie; Ren, Xinxin; Ge, Wei; Lin, Weigang \| 收藏 \| 浏览/下载：0/0 \| 提交时间：2023/06/16 Mixers (machinery) - Heat conduction - Manufacture