Design of multi-magnitude star simulation system based on adjustable background

[1]  H. Beutler.  The Theory of the Concave Grating , 1945 .

[2]  Christine Wall,et al.  Construction of a programmable light source for use as a display calibration artifact , 2001, IS&T/SPIE Electronic Imaging.

[3]  Steven W. Brown,et al.  LED-based spectrally tunable source for radiometric, photometric, and colorimetric applications , 2005 .

[4]  Zheng Xiao-bing.  Influence of spectrum not-matching on calibration precision of remote sensor , 2008 .

[5]  Liu Ze,et al.  Synthesis of Spectral Distribution for LED-based Source with Tunable Spectra , 2010 .

[6]  LI Ying-cai.  Design and performance analysis of standard starlight simulator , 2010 .

[7]  李宪圣 Li Xian-sheng,et al.  Spectrum-tunable Distribution and Spectral Matching for Integrating Sphere Light Source Based on Bromine Tungsten Lamps and LEDs , 2011 .

[8]  孙强 Sun Qiang,et al.  Design of astigmatism-free crossed Czerny-Turner spectrometer , 2012 .

[9]  李宪圣 Li Xian-sheng,et al.  Influence of Integrating Sphere Sources Distribution Temperature on Broadband Optical Remote Sensors Absolute Radiometric Calibration and Correcting Methods , 2012 .

[10]  倪国强 Ni Guoqiang,et al.  Design Method of Optical System of Improved Czerny-Turner Imaging Spectrometer , 2012 .

[11]  任建伟 Ren Jian-wei,et al.  LED-Based Single Star Simulator with Multi-Color-Temperature and Multi-Star-Magnitude Output , 2015 .

[12]  Xiao-Ni Li,et al.  The research of the light source for star simulator with automatic calibration and adjustable spectrum , 2015 .