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Chinese Academy of Sciences Institutional Repositories Grid
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Structural decomposition analysis of agricultural Non-CO2 greenhouse gas emission intensity in China 期刊论文  OAI收割
PHYSICS AND CHEMISTRY OF THE EARTH, 2024, 卷号: 134, 页码: 8
作者:  
Li, Minhuan;  Zhang, Fan;  Du, Yiqiong;  Zhang, Mengyi
  |  收藏  |  浏览/下载:22/0  |  提交时间:2024/07/24
Disentangling the effects of edaphic and vegetational properties on soil aggregate stability in riparian zones along a gradient of flooding stress 期刊论文  OAI收割
GEODERMA, 2021, 卷号: 385, 页码: 13
作者:  
Liu, Yan;  Ma, Maohua;  Ran, Yiguo;  Yi, Xuemei;  Wu, Shengjun
  |  收藏  |  浏览/下载:71/0  |  提交时间:2021/03/17
Image Inpainting Based on Structural Tensor Edge Intensity Model 期刊论文  OAI收割
International Journal of Automation and Computing, 2021, 卷号: 18, 期号: 2, 页码: 256-265
作者:  
Jing Wang, Yan-Hong Zhou, Hai-Feng Sima, Zhan-Qiang Huo, Ai-Zhong Mi
  |  收藏  |  浏览/下载:25/0  |  提交时间:2021/04/22
Coupling Structural Decomposition Analysis and Sensitivity Analysis to Investigate CO2 Emission Intensity in China 期刊论文  OAI收割
ENERGIES, 2019, 卷号: 12, 期号: 12, 页码: 23
作者:  
Li, Ling;  Tang, Ling;  Zhang, Junrong
  |  收藏  |  浏览/下载:48/0  |  提交时间:2020/01/10
Controlling factors for gas hydrate occurrence in Shenhu area on the northern slope of the South China Sea 期刊论文  OAI收割
science china-earth sciences, 2013, 卷号: 56, 期号: 4, 页码: 513-520
作者:  
Wang HongBin;  Yang ShengXiong;  Wu NengYou;  Zhang GuangXue;  Liang JinQiang
收藏  |  浏览/下载:25/0  |  提交时间:2016/10/26
Effect of thickness on the structural, electrical and optical properties of ZnO films deposited by MBE (EI CONFERENCE) 会议论文  OAI收割
2011 International Conference on Advanced Design and Manufacturing Engineering, ADME 2011, September 16, 2011 - September 18, 2011, Guangzhou, China
Yang X.; Su S.; Yi X.; Mei T.
收藏  |  浏览/下载:25/0  |  提交时间:2013/03/25
A set of ZnO films of different thickness have been deposited on sapphire substrates using molecular beam epitaxy (MBE) by varying the growth time and the effect of film thickness on the structural  electrical and optical properties have been investigated. The X-ray diffraction (XRD) results indicate that the full width at half maximum (FWHM) of the (002) diffraction peak is decreased as the film thickness increasing  and the stress along c-axis is stable. Scanning electron microscope (SEM) measurement shows that the grains become more uniform as the film grows thicker and the film surface present distinct hexagon shape as the film is grown up to a thickness of 500nm. The optical absorbance  Hall mobility and photoluminescence (PL) intensity are increased in accordance with the thickness of the film. (2011) Trans Tech Publications  Switzerland.  
Dynamic response of a single and a 4-bucket foundations 会议论文  OAI收割
7th International Conference on Physical Modelling in Geotechnics 2010, ICPMG 2010, Zurich, Switzerland, June 28, 2010 - July 1, 2010
作者:  
Zhang JH;  Zhang YM;  Lu XB(鲁晓兵)
收藏  |  浏览/下载:25/0  |  提交时间:2017/06/20
Energy-Level and Molecular Engineering of Organic D-pi-A Sensitizers in Dye-Sensitized Solar Cells 期刊论文  OAI收割
journal of physical chemistry c, 2008, 卷号: 112, 期号: 49, 页码: 19770-19776
Xu MF; Li RZ; Pootrakulchote N; Shi D; Guo J; Yi ZH; Zakeeruddin SM; Gratzel M; Wang P
收藏  |  浏览/下载:214/27  |  提交时间:2010/04/14
Using LMDI method to analyzed the change of China's industrial CO2 emissions from final fuel use: An empirical analysis 期刊论文  OAI收割
ENERGY POLICY, 2007, 卷号: 35, 期号: 11, 页码: 5892-5900
作者:  
Liu, Lan-Cui;  Fan, Ying;  Wu, Gang;  Wei, Yi-Ming
  |  收藏  |  浏览/下载:21/0  |  提交时间:2018/07/30
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:26/0  |  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.