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CAS IR Grid
机构
长春光学精密机械与物... [4]
国家天文台 [2]
西安光学精密机械研究... [2]
地理科学与资源研究所 [1]
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OAI收割 [11]
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期刊论文 [6]
会议论文 [4]
SCI/SSCI论文 [1]
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2020 [1]
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aircraft i... [1]
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Large aperture phase-coded diffractive lens for achromatic and 16° field-of-view imaging with high efficiency
期刊论文
OAI收割
Chinese Physics B, 2022, 卷号: 31, 期号: 7
作者:
Ma, Gu
;
Zheng, Peng-Lei
;
Hu, Zheng-Wen
;
Ma, Suo-Dong
;
Xu, Feng
  |  
收藏
  |  
浏览/下载:61/0
  |  
提交时间:2022/08/31
achromatic imaging
diffractive lens
phase coding
large aperture
high efficiency
Method to enhance the single mode fiber coupling efficiency for obscured receiver by beam shaping
期刊论文
OAI收割
Physica Scripta, 2020, 卷号: 95, 期号: 3
作者:
Rui, Daoman
;
Liu, Chao
;
Chen, Mo
;
Lan, Bin
;
Xian, Hao
  |  
收藏
  |  
浏览/下载:21/0
  |  
提交时间:2021/05/11
aperture obstruction
single-mode fiber
coupling efficiency
beam shaping
Optimization and Realization of Quadruple-Ridge Flared Horn With New Spline-Defined Profiles as a High-Efficiency Feed From 4.6 GHz to 24 GHz
期刊论文
OAI收割
IEEE TRANSACTIONS ON ANTENNAS AND PROPAGATION, 2019, 卷号: 67, 期号: 1, 页码: 585-590
作者:
Dong, Bin
;
Yang, Jian
;
Dahlstrom, Jens
;
Flygare, Jonas
;
Pantaleev, Miroslav
  |  
收藏
  |  
浏览/下载:11/0
  |  
提交时间:2020/03/10
Aperture efficiency
quadruple-ridge flared horn (QRFH)
sensitivity
spline-defined profiles
wideband feed
Experiments on the dish verification antenna china for the SKA
期刊论文
OAI收割
EXPERIMENTAL ASTRONOMY, 2016, 卷号: 42, 期号: 3, 页码: 301-317
作者:
Chai, Xiaoming
;
Liu, Bin
;
Yu, Lei
;
Yu, Shenghua
;
Wu, Di
  |  
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2019/04/08
Single-piece CFRP reflector
Pointing accuracy
Aperture efficiency
DVA-C
SKA
Experiments on the dish verification antenna china for the SKA
期刊论文
OAI收割
EXPERIMENTAL ASTRONOMY, 2016, 卷号: 42, 期号: 3, 页码: 301-317
作者:
Chai, Xiaoming
;
Liu, Bin
;
Yu, Lei
;
Yu, Shenghua
;
Wu, Di
收藏
  |  
浏览/下载:34/0
  |  
提交时间:2017/03/01
Single-piece CFRP reflector
Pointing accuracy
Aperture efficiency
DVA-C
SKA
Yb-doped large-mode-area aluminosilicate laser fibre fabricated by chelate precursor doping technique
期刊论文
OAI收割
electronics letters, 2016, 卷号: 52, 期号: 23, 页码: 1942-u42
作者:
Peng, Kun
;
Wang, Zhen
;
Zhan, Huan
;
Ni, Li
;
Gao, Cong
收藏
  |  
浏览/下载:122/0
  |  
提交时间:2016/11/22
ytterbium
aluminium compounds
doping
optical fibre fabrication
optical fibre testing
electron probe analysis
secondary ion mass spectroscopy
laser beams
optical fibre amplifiers
AlSiO:Yb
power 1 kW
efficiency 81
0 percent
slope efficiency
laser output
two-stage master oscillator power amplifier system
time-of-flight secondary ion mass spectrometry
electron probe microanalysis
fibre testing
numerical aperture
homogeneous large-core preform
gas flow control system
high-purity materials
chelate precursor doping technique
large mode area aluminosilicate laser fibre
Effects of experimental warming on stomatal traits in leaves of maize (Zea may L.)
SCI/SSCI论文
OAI收割
2013
作者:
Xu M.
;
Qiu S.
收藏
  |  
浏览/下载:95/0
  |  
提交时间:2014/12/24
Elevated temperature
maize (Zea may L.)
Ripley's K-function
spatial
distribution pattern
stomatal aperture size and shape
stomatal
frequency
radiation use efficiency
arabidopsis-thaliana
atmospheric co2
elevated co2
c-4 photosynthesis
leaf surface
drought susceptibility
adaptive significance
perennial grasses
abscisic-acid
Annular sub-aperture stitching interferometry for testing of large asphreical surfaces (EI CONFERENCE)
会议论文
OAI收割
International Symposium on Photoelectronic Detection and Imaging, ISPDI 2007: Optoelectronic System Design, Manufacturing, and Testings, September 9, 2007 - September 12, 2007, Beijing, China
作者:
Zheng L.-G.
;
Zhang X.-J.
;
Deng W.-J.
;
Wang X.-K.
收藏
  |  
浏览/下载:81/0
  |  
提交时间:2013/03/25
Annular subaperture stitching interferometric technology can test large-aperture
and the PV and RMS of residual error of the full aperture phase distribution is 0.027 and 0.0023
high numerical aperture aspheric surfaces with high resolution
the relative error of PV and RMS is -0.53% and -0.31%
respectively. The results conclude that this splicing model and algorithm are accurate and feasible. So it provides another quantitive measurement for test aspheric surfaces especially for large aperture aspheres besides null-compensation.
low cost and high efficiency without auxiliary null optics. In this paper
the basic principle and theory of the stitching method are introduced
the reasonable mathematical model and effective splicing algorithm are established based on simultaneous least-squares method and Zernike polynomial fitting. The translation errors are eliminated from each subaperture through the synthetical optimization stitching mode
it keeps the error from transmitting and accumulating. The numerical simulations have been carried on by this method. As results
the surface map of the full aperture after stitching is consistent to the input surface map
the difference of PV error and RMS error between them is -0.0074 and -0.00052 ( is 632.8nm)
respectively
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:36/0
  |  
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.
High power VCSEL device with periodic gain active region (EI CONFERENCE)
会议论文
OAI收割
Optoelectronic Materials and Devices II, November 2, 2007 - November 5, 2007, Wuhan, China
作者:
Zhang Y.
;
Liu Y.
;
Liu Y.
;
Liu Y.
;
Qin L.
收藏
  |  
浏览/下载:35/0
  |  
提交时间:2013/03/25
High power vertical cavity surface emitting lasers with large aperture have been fabricated through improving passivation
lateral oxidation and heat dissipation techniques. Different from conventional three quantum well structure
a periodic gain active region with nine quantum wells was incorporated into the VCSEL structure
with which high efficiency and high power operation were expected. The nine quantum wells were divided into three groups with each of them located at the antinodes of the cavity to enhance the coupling between the optical field and the gain region. Large aperture and bottom-emitting configuration was used to improve the beam quality and the heat dissipation. A maximum output power of 1.4W was demonstrated at CW operation for a 400m-diameter device. The lasing wavelength shifted to 995.5nm with a FWHM of 2nm at a current of 4.8A due to the internal heating and the absence of active water cooling. A ring-shape farfield pattern was induced by the non-homogeneous lateral current distribution in large diameter device. The light intensity at the center of the ring increased with increasing current. A symmetric round light spot at the center and single transverse mode operation with a divergence angle of 16 were observed with current beyond 4.8A.