The simulation of intra-pixel sensitivity for HgCdTe infrared focal plane array

被引:1
作者
Zhong Li [1 ,3 ]
Su Xiao-Feng [1 ]
Hu Wei-Da [1 ]
Chen Fan-Sheng [1 ,2 ]
机构
[1] Chinese Acad Sci, Shanghai Inst Tech Phys, Key Lab Intelligent Infrared Percept, Shanghai 200083, Peoples R China
[2] Univ Chinese Acad Sci, Hangzhou Inst Adv Study, Hangzhou 310024, Peoples R China
[3] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
基金
中国国家自然科学基金;
关键词
intra-pixel sensitivity; HgCdTe; infrared focal plane array; non-uniformity; Monte Carlo Method; MODULATION TRANSFER-FUNCTION; SMALL-PITCH; CROSSTALK;
D O I
10.11972/j.issn.1001-9014.2021.05.014
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
For the under-sampled imaging infrared search and tracking system which F lambda/d<2, the energy of point target was concentrated on a single pixel. Due to the spatial non-uniformity of intra-pixel sensitivity (IPS) for focal plane array, the calculation accuracy of energy and centroid for point target would be reduced. Light spot scanning test and numerical simulation could effectively characterize and analyze the IPS. but the system and model were highly complex and time-consuming, moreover, experimental tests couldn't analyze the relationship between the spatial non-uniformity of the IPS and the parameters of photo-detector. Aimed at the above problem, Monte Carlo methods were used to simulate the IPS of HgCdTe infrared focal plane array, and the influencing factors of its spatial non-uniformity were analyzed. The results showed that the spatial non-uniformity of IPS can be reduced by reducing the pixel pitch or increasing the thickness of absorber. With the increased in wavelength, the spatial non-uniformity of IPS increased slightly. The results of simulation and analysis are of great significance for improving the measurement accuracy of high energy concentration point target.
引用
收藏
页码:673 / 679
页数:7
相关论文
共 24 条
[1]   Toward high-precision astrometry with WFPC2. I. Deriving an accurate point-spread function [J].
Anderson, J ;
King, IR .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2000, 112 (776) :1360-1382
[2]   Parametric numerical study of the modulation transfer function in small-pitch InGaAs/InP infrared arrays with refractive microlenses [J].
Appleton, Brian ;
Hubbard, Taylor ;
Glasmann, Andreu ;
Bellotti, Enrico .
OPTICS EXPRESS, 2018, 26 (05) :5310-5326
[3]   Subpixel response measurement of near-infrared detectors [J].
Barron, N. ;
Borysow, M. ;
Beyerlein, K. ;
Brown, M. ;
Lorenzon, W. ;
Schubnell, M. ;
Tarle, G. ;
Tomasch, A. ;
Weaverdyck, C. .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2007, 119 (854) :466-475
[4]   Modeling and Characterization of MTF and Spectral Response at Small Pitch on Mercury Cadmium Telluride [J].
Berthoz, J. ;
Grille, R. ;
Rubaldo, L. ;
Gravrand, O. ;
Kerlain, A. ;
Pere-Laperne, N. ;
Martineau, L. ;
Chabuel, F. ;
Leclercq, D. .
JOURNAL OF ELECTRONIC MATERIALS, 2015, 44 (09) :3157-3162
[5]   EMPIRICAL RULE OF INTRINSIC ABSORPTION-SPECTROSCOPY IN HG1-XCDXTE [J].
CHU, JH ;
LI, B ;
LIU, K ;
TANG, DY .
JOURNAL OF APPLIED PHYSICS, 1994, 75 (02) :1234-1235
[6]  
FASTOW R, 1994, P SOC PHOTO-OPT INS, V2274, P136, DOI 10.1117/12.189239
[7]   Detection and measurement of poorly sampled point sources imaged with 2-D arrays [J].
Howell, SB ;
Koehn, B ;
Bowell, E ;
Hoffman, M .
ASTRONOMICAL JOURNAL, 1996, 112 (03) :1302-1311
[8]   Subpixel sensitivity map for a charge-coupled device sensor [J].
Kavaldjiev, D ;
Ninkov, Z .
OPTICAL ENGINEERING, 1998, 37 (03) :948-954
[9]   A new technique of characterization of intrapixel response dedicated to astronomical detectors [J].
Ketchazo, C. ;
Viale, T. ;
Boulade, O. ;
Druart, G. ;
Moreau, V. ;
Mugnier, L. ;
Dubrueil, D. ;
Derelle, S. ;
Ronayette, S. ;
Guerineau, N. ;
Berthe, M. .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2015, 787 :265-269
[10]  
Ketchazo C, 2017, INT C SPAC OPT PHOT, V10562