Registration and restoration of Adaptive-Optics corrected retinal images

L. Blanco, L. Mugnier, A. Bonnefois, M. Pâques
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引用次数: 6

Abstract

Raw individual Adaptive-Optics-corrected flood-illuminated retinal images are usually quite noisy because of safety flux limitations. These flood-illuminated images are also of poor contrast. Interpretation of such images is therefore difficult without an appropriate post-processing, which typically includes the registration of the recorded image stack into a mosaic image and the restoration of the latter.We have developed an image registration method in a MAP framework, based on previous work in astronomical imaging, and tailored for the specifics of retinal imaging, more precisely to the fact that the illumination of the retina and the transmission of the instrument is non-homogeneous, which makes conventional registration methods likely to fail. The mosaic image must then be deconvolved in order to visually restore the high-resolution brought by adaptive optics. To this aim, we perform an unsupervised myopic deconvolution that takes into account the 3D nature of the object being imaged. We successfully apply this whole processing chain to experimental in vivo images of retinal vessels.
自适应光学校正视网膜图像的配准与恢复
由于安全通量的限制,原始的个体自适应光学校正的泛光视网膜图像通常相当嘈杂。这些被洪水照亮的图像对比度也很差。因此,如果没有适当的后处理,解释这种图像是困难的,后处理通常包括将记录的图像堆栈配准到马赛克图像中并恢复后者。我们在MAP框架中开发了一种图像配准方法,该方法基于先前在天文成像方面的工作,并针对视网膜成像的具体情况进行了定制,更精确地考虑到视网膜的照明和仪器的传输是不均匀的,这使得传统的配准方法可能失败。然后必须对拼接图像进行反卷积,以便在视觉上恢复自适应光学带来的高分辨率。为此,我们执行了无监督的近视反卷积,考虑到被成像物体的3D性质。我们成功地将整个处理链应用于视网膜血管的实验体内图像。
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