由多个小口径成像系统通过特殊排列综合而成的光学稀疏孔径系统是实现高分辨率天文目标成像观测的一种新方法。
Optical sparse-aperture system can be designed to obtain high resolution in astronomical object imaging. It is a particular array synthesized by several small filled imaging systems.
选型时要根据扫描仪的光学分辨率、色位数、品牌、价格等因素综合考虑。
It should be considered comprehensively with respect to the factors of optical resolution of scanner, color bits, brand and price.
综合应用窄带子波记录及重构记录的不同分辨率特征，可以有效地识别某些细薄的隐蔽圈闭。
Some very thin subtle traps can be recognized effectively with the help of different resolution character of narrow band wavelet record and reconstructed record.
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