• 摘要: 衍射成像技术在遥感成像、生物微观观测、材料结构分析等领域应用广泛,是依托光的衍射特性,通过观测得到的衍射图像与点扩散函数(point spread function, PSF)反卷积重建物体信息的先进光学成像技术。但实际观测点扩散函数易受成像系统光学元件缺陷、探测器噪声等因素的干扰,与真实PSF之间存在误差,进而导致衍射成像效果不佳,故研究PSF修正技术意义重大。经过充分调查与研究国内外相关文献后,本文首先总结分析因成像元件固有限制、动态干扰和复杂场景等多种因素导致PSF退化的原因。进而梳理从多目标融合调制传递函数(modulation transfer function, MTF)模型结合算法、PSF建模等光学硬件与传统计算算法的修正方式,到相位掩模优化网络、BGnet等深度学习与数据驱动方法的PSF修正方法发展历程。这些方法均为PSF不同使用场景的修正提供了解决方案。最后介绍在图像、天文与空间成像、生物医学成像等领域中的PSF修正技术应用情况。随着学科交叉融合与相关技术的发展,PSF修正技术将为天体探测、微观结构观测等领域提供更有力的支撑。

       

      Abstract: Diffractive imaging technology, widely applied in remote sensing imaging, biological microscopic observation and material structure analysis, is an advanced optical imaging technology that reconstructs object information via deconvolution of observation-derived diffraction images with the point spread function (PSF). However, the actually measured PSF is prone to interference from imaging system optical component defects and detector noise, leading to discrepancies from the true PSF and thus degraded diffractive imaging performance. Therefore, the research on PSF correction technology is of great significance.After a comprehensive review of domestic and international literature, this paper first summarizes and analyzes the causes of PSF degradation, including inherent limitations of imaging components, dynamic interference, and complex scenarios. It then traces the evolution of PSF correction methods, ranging from optical hardware and traditional computational algorithms (such as modulation transfer function (MTF)-based fusion models and PSF modeling) to deep learning and data-driven approaches (including phase mask optimization networks and BGnet). These methods provide solutions for PSF correction in various application scenarios. Finally, the paper introduces the application of PSF correction techniques in fields such as image processing, astronomical and space imaging, and biomedical imaging. In the future, with interdisciplinary integration and advancements in related technologies, PSF correction techniques will offer stronger support for areas like celestial exploration and microscopic structural observation.