中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
机构
采集方式
内容类型
发表日期
学科主题
筛选

浏览/检索结果: 共10条,第1-10条 帮助

条数/页: 排序方式:
Potassium-Promoted Three-Dimensional Mesoporous Pt/MnO2 for Formaldehyde Elimination at Zero Degree 期刊论文  OAI收割
JOURNAL OF THE CHEMICAL SOCIETY OF PAKISTAN, 2020, 卷号: 42, 期号: 2, 页码: 188-203
作者:  
Guan, Shengnan;  Li, Wenzhi;  Ma, Jianru;  Liu, Qingchuan;  Chen, Kun
  |  收藏  |  浏览/下载:21/0  |  提交时间:2020/10/29
The design of the force actuator used in extreme low temperature environment 会议论文  OAI收割
Montréal, Quebec, Canada, 2014-6-22
作者:  
Yu Ye;  Bozhong Gu;  Xiaolong Han
收藏  |  浏览/下载:32/0  |  提交时间:2015/03/13
Analysis, testing and control of telescope’s high-precision drive system in low-temperature environment 会议论文  OAI收割
Montréal, Quebec, Canada, 2014-6-22
作者:  
DU Fu-Jia;  WEN Hai-Kun;  ZHANG Jian
收藏  |  浏览/下载:34/0  |  提交时间:2015/03/12
A study of the evolution of rust on weathering steel submitted to the Qinghai salt lake atmospheric corrosion 期刊论文  OAI收割
Materials Chemistry and Physics, 2013, 卷号: 139, 期号: 1, 页码: 225-232
J. Wang; Z. Y. Wang; W. Ke
收藏  |  浏览/下载:12/0  |  提交时间:2013/12/24
Highly expanded flashing liquid jets in vacuum environment 会议论文  OAI收割
Beijing, China, September 23, 2013 - September 27, 2013
作者:  
Du WF(杜王芳);  Zhao JF(赵建福)
  |  收藏  |  浏览/下载:30/0  |  提交时间:2018/11/08
Design and experimental research of a new type focus mechanism used in space-based 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:  
Wang D.
收藏  |  浏览/下载:40/0  |  提交时间:2013/03/25
The position of focal plane will be changed because of temperature fluctuation and vacuum environment. In order to make the telescope work well  positioning accuracy of the mechanism is 0.008mm. The performance satisfies the need of precision  a focusing mechanism is needed. To majority of large space-based telescopes  and the scheme design is reasonable and practicable. 2012 IEEE.  the general way to do this would be to use a reflector  which was located in the backfocal distance. One of typical schemes of this mechanism was introduced  however  because of the big axial size  the mechanism can't be used when the size of the enclosure was limited. A new type of focusing mechanism was introduced  which has such advantages of small size  high accuracy and low mass. The design and test methods had been discussed. According to the results  the repeatability positioning accuracy is 0.0025mm  
Characterisation of rust formed on carbon steel after exposure to open atmosphere in Qinghai salt lake region 期刊论文  OAI收割
Corrosion Engineering Science and Technology, 2012, 卷号: 47, 期号: 2, 页码: 125-130
J. Wang; Z. Y. Wang; W. Ke
收藏  |  浏览/下载:43/0  |  提交时间:2013/02/05
Design and test of focusing mechanism of space camera (EI CONFERENCE) 会议论文  OAI收割
5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Design, Manufacturing, and Testing of Micro- and Nano-Optical Devices and Systems, April 26, 2010 - April 29, 2010, Dalian, China
作者:  
Li Y.;  Li Y.;  Li Y.;  Wang H.;  Wang H.
收藏  |  浏览/下载:33/0  |  提交时间:2013/03/25
According to the focal depth and work environment of a space camera  a focusing mechanism is designed  which consists of precision screw ball transmission and linear bearing guidance and accuracy improving. The dynamic- strike- resistance  adaptability to temperature and vacuum are considered into the reliable design method. Furthermore  the linearity error  the structure stability and the mechanism work situation in high and low temperature are tested. The result is that the linearity error of the mechanism is less than 0.003 mm  and the sway error of vertical way and level way of the mirror is less than 20''. The linearity error of the mechanism and the sway error of the mirror remain unchanged after vibration test. The mechanism can work in the complex space environment. 2010 SPIE.  
Corrosion behaviour of weathering steel in diluted Qinghai salt lake water in a laboratory accelerated test that involved cyclic wet/dry conditions 期刊论文  OAI收割
Materials Chemistry and Physics, 2010, 卷号: 124, 期号: 2-3, 页码: 952-958
J. Wang; Z. Y. Wang; W. Ke
收藏  |  浏览/下载:17/0  |  提交时间:2012/04/13
The calibration of faint simulation star magnitude based on single photon count technique (EI CONFERENCE) 会议论文  OAI收割
International Symposium on Photoelectronic Detection and Imaging 2009: Advances in Imaging Detectors and Applications, June 17, 2009 - June 19, 2009, Beijing, China
作者:  
Xu S.-Y.;  Guo J.;  Guo J.
收藏  |  浏览/下载:35/0  |  提交时间:2013/03/25
A calibration method of faint star magnitude of the star scene simulation device is proposed in this paper. In the research of simulation star magnitude  luminometers and CCD devices are the general calibration devices which are used to measure the illumination intensity and calibrate its magnitude. But if the simulation magnitude is only sixth magnitude  its illumination intensity is only 1.010-8 Lux. This illumination intensity level is the lowest illumination intensity that the commercial luminometer can detect. Hence the simulation star magnitude lower than six magnitude cannot be calibrated by luminoters. Likewise CCD devices also need an additive cooler in this case. When the single photon characteristic is presented due to the low luminosity of simulating light sources  the simulation star magnitude can be calibrated by detecting its photon flux of radiation with the method of single photon count. In this paper the detection principle of single photon based on a compact designed PMT detecting of the radiation level of simulation star magnitude is advanced. Especially a spectrum match method is proved theoretically to be an effective means for selecting PMT photosensitive type. In the case of the detection object of the simulation star in visible wavelength  a analysis indicates that the material of tri-alkali cathode materials its best choice after being compared the Signal-to-Noise of photon detector of several PMT photosensitive materials based on the different spectrum match ratio of different object light sources and different cathode materials. An experiment is employed to show the relationship of control voltage of PMT and its dark counter  the relationship of the environment temperature of PMT and its dark counter  which proves its only decades of CPS at room temperature. The so low dark counter avoids a bulky cooler and is convenient for installing it on the star scene simulation equipment. Finally in the experiment of calibrating the simulation star magnitudes the ability of its calibration is confirmed to reaches up to 12m  meanwhile its calibration error is within 0.2m. 2009 SPIE.