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Photon Counting Imaging with Low Noise and a Wide Dynamic Range for Aurora Observations 期刊论文
Sensors, 2020, 卷号: 20, 期号: 20, 页码: 21
作者:  Z. W. Han,K. F. Song,H. J. Zhang,M. Yu,L. P. He,Q. F. Guo,X. Wang,Y. Liu and B. Chen
收藏  |  浏览/下载:2/0  |  提交时间:2021/07/06
Inductive Charge Readout for Far Ultraviolet Photon Count Imaging Detector 期刊论文
Guangzi Xuebao/Acta Photonica Sinica, 2020, 卷号: 49, 期号: 7
作者:  K.-F. Song,Z.-W. Han,L.-P. He and Q.-L. Ni
收藏  |  浏览/下载:2/0  |  提交时间:2021/07/06
A novel model for calculating the inter-electrode capacitance of wedge-strip anode 期刊论文
Review of Scientific Instruments, 2016, 卷号: 87, 期号: 4
作者:  Zhao, A. R. and Q. L. Ni
收藏  |  浏览/下载:14/0  |  提交时间:2017/09/11
Swing arm profilometer: analytical solutions of misalignment errors for testing axisymmetric optics 期刊论文
Optical Engineering, 2016, 卷号: 55, 期号: 7
作者:  Xiong, L.;  X. Luo;  Z. Y. Liu;  X. K. Wang;  H. X. Hu
收藏  |  浏览/下载:22/0  |  提交时间:2017/09/11
短脉冲激光烧蚀理论及楔条形阳极加工方法研究 学位论文
博士: 中国科学院大学, 2015
作者:  金方圆
收藏  |  浏览/下载:38/0  |  提交时间:2015/11/30
Curved focal plane extreme ultraviolet detector array for a EUV camera on CHANG E lander 期刊论文
Optics Express, 2015, 卷号: 23, 期号: 24, 页码: 30755-30766
作者:  Ni, Q.;  K. Song;  S. Liu;  L. He;  B. Chen and W. Yu
收藏  |  浏览/下载:15/0  |  提交时间:2016/07/15
Vernier Anode Design and Image Simulation 期刊论文
Spectroscopy and Spectral Analysis, 2015, 卷号: 35, 期号: 12
作者:  A. R. Zhao;  Q. L. Ni and K. F. Song
收藏  |  浏览/下载:13/0  |  提交时间:2016/08/04
Optimization for spatial resolution and count rate of a far ultraviolet photon-counting imaging detector based on induced charge position-sensitive anode 期刊论文
Guangxue Xuebao/Acta Optica Sinica, 2014, 卷号: 34, 期号: 8
Ni Q.
收藏  |  浏览/下载:15/0  |  提交时间:2015/04/24
The characteristic performance of an extreme ultraviolet MCP-based photon-counting imaging detector 会议论文
5th International Symposium on Photoelectronic Detection and Imaging, ISPDI 2013, June 25, 2013 - June 27, 2013, Beijing, China
Ni Q.; Song K.
收藏  |  浏览/下载:16/0  |  提交时间:2014/05/15
Study on spectrograph for ionosphere: A broadband imaging instrument prototype for far-ultraviolet (EI CONFERENCE) 会议论文
International Symposium on Photoelectronic Detection and Imaging 2011: Space Exploration Technologies and Applications, May 24, 2011 - May 26, 2011, Beijing, China
Yu L.; Wang S.-R.; Lin G.-Y.
收藏  |  浏览/下载:20/0  |  提交时间:2013/03/25
Current research on space-based exploration for the ionosphere needs more advanced technologies. Because the spectral signals in the ionosphere distributing basically in the far-ultraviolet waveband are very weak. Usual spectrometer structures and detectors such as CCD can't receive enough information. Based on this principle of atmospheric sounding  the imaging spectrometer prototype for ionosphere detection application was designed to solve the problem. This prototype consists of the telescope and the imaging spectrometer. The simple structure and small number of mirrors can help higher transmission efficiency be achieved and weak signals detection be implemented. The telescope is an off-axis parabolic mirror and the spectrometer is a modified Czerny-Turner spectral imaging system. Modified Czerny-Turner spectrometer contains a spherical mirror  a fixed plane grating and a toroidal mirror. By adjusting the incident angle to the collimating mirror and using toroidal mirror  coma and astigmatism were corrected well. We also optimize distances between the grating to the focusing mirror and the focusing mirror to the image plane to improve disadvantages of traditional Czerny-Turner structure. Designed results demonstrate that aberrations are substantially corrected  and high image quality can be obtained in broad waveband. The photon counting Wedge-Strip-Anode detector with micro-channel planes as the receiving plane is accepted for the instrument prototype. The other photon counting 2-D detector responding well for weak light such as Cross-Delay line detector and MAMA detector can also be used for detection. The calibration and performances testing system is made of a vacuum system  a deuterium lamp  a monochrometer and the instrument prototype. Results obtained from the experiment show that the spectral resolution is 2.4 nm and the spatial resolution is 80 m. The other calibration experiments are running. The technology of the spectrometer prototype is important for the research and applications of ionosphere remote sensing. 2011 SPIE.  


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