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长春光学精密机械与物... [2]
清华大学 [1]
厦门大学 [1]
西安交通大学 [1]
内容类型
会议论文 [2]
期刊论文 [2]
学位论文 [1]
发表日期
2011 [1]
2010 [2]
2007 [1]
2004 [1]
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The investigation of point defect modes of phononic crystal for high Q resonance (EI CONFERENCE)
会议论文
2011 16th International Solid-State Sensors, Actuators and Microsystems Conference, TRANSDUCERS'11, June 5, 2011 - June 9, 2011, Beijing, China
Li F.
;
Liu J.
;
Wu Y. H.
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浏览/下载:17/0
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提交时间:2013/03/25
Point defect cavity was constructed in a two-dimensional phononic crystal plate. It was excited by a small piezo chip in the cavity and the vibration of each point defect modes were detected by an optical interferometer. Point defect modes on 2D PC plate in vacuum
air and loaded with water were investigated theoretically and experimentally to make clear of Q factors
which are affected by inner attenuation
band gap effects and medium. The way to get high Q resonance has been found. It helps to design a new kind of resonator or sensor. 2011 IEEE.
中学教师的工作满意度状况及其相关因素
期刊论文
2010, 2010
孙汉银
;
李虹
;
林崇德
;
Sun Hanyin
;
Li Hong
;
Lin Chongde
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浏览/下载:2/0
Study on the frequency band for interpolation method used in distributed parameter line model
期刊论文
Zhongguo Dianji Gongcheng Xuebao/Proceedings of the Chinese Society of Electrical Engineering, 2010, 卷号: 30, 期号: [db:dc_citation_issue], 页码: 72-76
作者:
Song, Guo-Bing
;
Liu, Lin-Lin
;
Suonan, Jia-Le
;
Zhao, Xuan-Zong
;
Zhang, Jun-Min
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浏览/下载:3/0
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提交时间:2019/12/10
Affected factors
Current distribution
Distributed parameter
Distributed parameter line model
Interpolation method
Linear Interpolation
Periodic signal
Sampling frequencies
Research on the support structure of the primary mirror of large-aperture telescope (EI CONFERENCE)
会议论文
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.
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浏览/下载:22/0
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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.
我国电力市场价格形成机制研究
学位论文
2004, 2004
戴平生
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浏览/下载:2/0
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提交时间:2016/02/14
电价形成
影响因素
市场方法
electricity price forming
affected factors
markets method
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