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CAS IR Grid
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长春光学精密机械与物... [9]
中国科学院大学 [1]
近代物理研究所 [1]
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会议论文 [8]
期刊论文 [3]
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The design of atmosphere polarimetry sensing with multi-bands
期刊论文
OAI收割
Optics Communications, 2018, 卷号: 410, 页码: 863-866
作者:
Dou, C. H.
;
Wang, S. R.
;
Zhang, Z. H.
;
Huang, Y.
;
Yang, X. H.
  |  
收藏
  |  
浏览/下载:21/0
  |  
提交时间:2019/09/17
Polarimetric imaging
Geometric optical design
Remote sensing and
sensors
Lens system design
cloud
Optics
High energy electron radiography system design and simulation study of beam angle-position correlation and aperture effect on the images
期刊论文
OAI收割
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2016, 卷号: 832, 页码: 144-151
作者:
Zhao, Y. T.
;
Gai, W.
;
Du, Y. C.
;
Zhao, Quantang
  |  
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2018/05/31
High energy electron radiography
Imaging lens system
Linear achromat
Angle-position correlation
High energy electron radiography system design and simulation study of beam angle-position correlation and aperture effect on the images
期刊论文
iSwitch采集
Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment, 2016, 卷号: 832, 页码: 144-151
作者:
Zhao, Quantang
;
Cao, S. C.
;
Liu, M.
;
Sheng, X. K.
;
Wang, Y. R.
收藏
  |  
浏览/下载:42/0
  |  
提交时间:2019/05/09
High energy electron radiography
Imaging lens system
Linear achromat
Angle-position correlation
Design and analysis of auto-focus assembly for spaceborne remote sensing camera (EI CONFERENCE)
会议论文
OAI收割
2011 International Conference on Electronics, Communications and Control, ICECC 2011, September 9, 2011 - September 11, 2011, Ningbo, China
作者:
Chen W.
;
Gao X.
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2013/03/25
Spaceborne remote sensing camera may be out of focus when the environment and photographic distance changes. In order to get higher ground sampled distance for the camera
based on the experience gained from the development of a remote sensing camera
working principle of auto-focus assembly control system was discussed. Time of waveform extraction was reduced. It sets force an auto-focus assembly that uses cam and line guide rail in order to move the lens group. The motion error of the auto-focus assembly was difficult to be eliminated and would affect on the focusing accuracy of the spaceborne remote sensing camera directly. So it was analyzed at both ends of the focusing structure. The CCD detector can keep stable when the remote sensing camera is imaging. The motion error was tested to verify the validity of the simulation result and it is less than 0.01mm. Its accuracy meets using demand. The focusing method of moving focal plane is suitable for spaceborne remote sensing camera. 2011 IEEE.
Optical system of golay-3 synthetic aperture telescope of Fizeau style (EI CONFERENCE)
会议论文
OAI收割
2010 3rd International Conference on Advanced Computer Theory and Engineering, ICACTE 2010, August 20, 2010 - August 22, 2010, Chengdu, China
作者:
Sun Z.-Y.
收藏
  |  
浏览/下载:19/0
  |  
提交时间:2013/03/25
In order to get high resolution
the field of view is 4. Analyzed the imaging
a optical system of golay-3 synthetic aperture telescope has been designed which adopt Fizeau multi-telescope frame. The angular magnification of sub-aperture is -4
the fill factor is 113. The configuration of light beam combiner is Cassegrain style added a lens. The total focal length is 6000mm
the PSF have been improved remarkably
and the cut-off frequency of MTF is close to that of full aperture. 2010 IEEE.
Thermal difference analysis and athermalization design of infrared optical system (EI CONFERENCE)
会议论文
OAI收割
Optical Design and Testing IV, October 18, 2010 - October 20, 2010, Beijing, China
作者:
Zhang X.
;
Zhang X.
;
Zhang X.
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2013/03/25
When infrared optical system works in a large temperature range
the thermal effect of optical lens and optical tube will produce image plane shift and lead to imaging quality deterioration. In order to eliminate the thermal aberration
the athermalization design principles of infrared optical system were introduced
and some commonly used methods of thermal difference compensation were described. Proceeding from single lens
the thermal difference caused by temperature changing was analyzed
and the relationship between temperature and focus shift was obtained. Considering optical tube thermal expansion
a set of equations to estimate the thermal difference of lens group was given. Finally
an infrared optical imaging system that can work under the temperature range of -40C to 60C was design according to athermal technique
in which a new mechanical passive temperature compensation was proposed. Through simulation
the athermalization design could make imaging plane shift the smallest. The simulation results coincided with the theoretical formula
and the design had reference value in engineering. 2010 Copyright SPIE - The International Society for Optical Engineering.
Development and radiance calibration of three-waveband camera (EI CONFERENCE)
会议论文
OAI收割
International Symposium on Photonics and Optoelectronics, SOPO 2010, June 19, 2010 - June 21, 2010, Chengdu, China
作者:
Wang J.
;
Liu Y.
;
Liu Y.
;
Sun Q.
;
Liu Y.
收藏
  |  
浏览/下载:29/0
  |  
提交时间:2013/03/25
An imaging system with three-waveband sharing one lens and an area CCD was developed. By rotating different filters into the beam path
the required waveband was selected. The optical system which can image in ultraviolet
visible and near infrared region was designed and the signal collecting system was integrated. The optical design and system integration have some advantages such as low cost
small size and light in weight. To obtain a high imaging quality
the radiation calibration is carried out in order to establish the relation between the average grey level of output image and the input radiance from the integrating sphere. According to the calibration data in experiments
the radiation dynamic range and the best working point of the system are determined. The experiment result shows that the dynamic range of the image system is maximal when the exposure time is 8ms in ultraviolet
0.5ms in visible and 0.125ms in near infrared region. 2010 IEEE.
Design of high-resolution fourier transform lens (EI CONFERENCE)
会议论文
OAI收割
3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Advanced Optical Manufacturing Technologies, July 8, 2007 - July 12, 2007, Chengdu, China
作者:
Zhang L.
;
Zhang L.
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2013/03/25
With the development of optical information processing
high-resolution Fourier transform lens has often been used in holographic data storage system
spatial filtering and observation of particles. This paper studies the optical design method of high-resolution Fourier transform optical lenses system
which could be used in particles observation and holographic data storage system. According to Fourier transform relation between object and its frequency plane and the theory of geometrical optics
the system with working wavelength 532nm and resolution 3 m was designed based on ZEMAX. A multi-configuration method was adopted to optimize the system's lenses. In the optical system
a diaphragm was placed at the system's spectrum plane and the system demanded a low vacuum to cut down the influences of atmosphere and other particles. The result of finite element analysis indicated that the influences of vacuum pumping to optics spacing and mirror surface shape very minor
and the imaging quality not being affected. This system has many advantages
such as simple structure
good image quality and a high resolution of 3 m. So it has a wide application prospect and can be used both in holographic data storage system and particles observation.
Design of dual-FOV refractive/diffractive LWIR optical system (EI CONFERENCE)
会议论文
OAI收割
3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Advanced Optical Manufacturing Technologies, July 8, 2007 - July 12, 2007, Chengdu, China
作者:
Wang L.-J.
;
Zhang J.-P.
;
Wang L.-J.
;
Zhang X.
;
Zhang X.
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2013/03/25
An infrared-optical zoom system using binary element is proposed in this paper. The two main advantages of the zoom system introducing here are: bigger F-number and lower cost. The primary optical properties are: F/#=1
Second
Others
zoom ratio =1:4
binary element is used to correct the chromatical aberration by taking the advantage of negative dispersion characteristics and the cost of the system is lower than that of conventional ones with Zinc Selenide (Znse) material at the same level. In the binary element is rotational symmetric with one step which is easy to fabricate
in order to balance 5th spherical aberration
and dual field are 26.6 and 5.6respectively. Wider field of view is used for search and the smaller one is used for imaging details. This system uses un-cooled infrared detector with 320240 pixels and 45m pixel size. The F-number matches the sensitivity range of the detector array. Three aspects are considered during design process to make the system more satisfactory and more achievable. First
5th coma aberration and 5th astigmatic aberration
the manner of zoom is accomplished by exchanging tow lenses into the smaller field of view system layout. The lens exchange manner faces the requirement of simple system structure and good image quality in both focal points. It can also make the system more feasible in the alignment process than mechanical-zooming manner and optical-zooming manner
high-order asphere surfaces with 2th order to 10 th order are also hired in the system. Asphere surface is useful in compressing the system and improving optical system transmittance. This kind asphere surface is on industrial level featuring low cost and easy to fabricate. It is shown that good image quality can achieved by implementing five Germanium lenses and the transmittance of system is 72%. All aberrations are diffraction-limited
both spherical aberration and astigmatic aberration are corrected. When the field of view(FOV) is 26.6 and the focal length is 152mm
MTF at Nyquist frequency(11lp/mm) is great than 0.7. The spherical aberration is -0.0073. The coma aberration is 0.0978 and the astigmatic aberration is -0.013. When the field of view(FOV) is 5.6 and the focal length is 38mm
MTF at Nyquist frequency is great than 0.8 with spherical aberration -0.0046
the coma aberration 0.055 and astigmatic aberration 0.034.
Self Imaging technique for refocusing an aerospace camera (EI CONFERENCE)
会议论文
OAI收割
ICO20: Optical Devices and Instruments, August 21, 2005 - August 26, 2005, Changchun, China
作者:
Li W.
;
Li W.
;
Wang X.
;
Wang X.
;
Wang X.
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2013/03/25
A novel auto-focusing technique using a self imaging approach is developed for an aerospace camera having large aperture and long focus. Its optical system consists of an emitting system
receiving system
and two penta-prisms. Emitting system has three parts: a light source
beamsplitter
and aim slit. The receiving system includes a field lens
two separate lenses
and CCD. Using two little penta-prisms instead of a large planar mirror makes the autofocus system simple and compact. CCD was used as photoelectric converting device. A defocused signal is acquired by measuring the change of the two slit self-images position imaged on the CCD. A simple and compact construction of the auto-focusing system was proposed. The algorithm to calculate the moving of the slit-self images position was analyzed in order to achieve subpixel position estimation. The results of the experiments show a 10m focusing precision. The system demonstrates high resolution
easy adjustment and high reliability.