Jiang Yuesong, Zhang Jingjing, He Yuntao, Wang Haiyang, Wang Jing, Zhang Jun
School of Electronic and Information Engineering, Beihang University, Beijing 100191, China.
J Opt Soc Am A Opt Image Sci Vis. 2012 Mar 1;29(3):295-302. doi: 10.1364/JOSAA.29.000295.
The fractional Fourier transform, which is a generalization of the classical Fourier transform, is introduced into an optical aperture synthesis (OAS) system by which imaging of an astronomical object can be achieved. We introduce fractional Fourier optical imaging and fractional Fourier-domain filtering (FFDF), and then present the schematic diagram of an OAS imaging system with FFDF. The modulation transfer function of an OAS system with FFDF is compared with that of an OAS system in the same condition. The result indicates that the OAS system with FFDF has larger practical cutoff frequency when the fill factor is smaller. Furthermore, the quality of imaging and restoration also demonstrates this conclusion.
分数傅里叶变换是经典傅里叶变换的推广,被引入到光学孔径合成(OAS)系统中,通过该系统可以实现天文物体的成像。我们介绍了分数傅里叶光学成像和分数傅里叶域滤波(FFDF),然后给出了具有FFDF的OAS成像系统的示意图。将具有FFDF的OAS系统的调制传递函数与相同条件下的OAS系统的调制传递函数进行了比较。结果表明,当填充因子较小时,具有FFDF的OAS系统具有更大的实际截止频率。此外,成像和恢复的质量也证明了这一结论。