优化用于非相干 HiLo 显微镜的微透镜阵列

Q3 Physics and Astronomy
Ziao Jiao , Xi Chen , David Day Uei Li
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引用次数: 0

摘要

HiLo 显微镜是一种功能强大、成本低廉且易于配置的技术,可用于获取高对比度的光学切片图像。然而,传统的 HiLo 显微镜基于带有扩散玻璃板的相干光源或带有数字镜像设备(DMD)和空间光调制器(SLM)的非相干光源,这些设备都比较昂贵。在这里,我们提出了一种使用工作重点和非相干 LED 光源的新型低成本 HiLo 显微镜技术。我们模拟了结构照明(SI)模式和 HiLo 图像生成。为了观察 MLA 对 HiLo 图像的影响,我们使用了三种具有特定微透镜间距和数值孔径 (NA) 的普通 MLA 来生成周期性照明模式。模拟结果表明,MLA 的 NA 对 HiLo 图像的影响不大,而较大的透镜间距可以带来更高的图像对比度。不过,镜头间距有一个最佳值。如果透镜间距等于或大于 140 μm,HiLo 图像中就会出现伪影。根据我们的模拟,采用 0.01NA 和周期为 120 μm 的十字型 MLA 可获得最佳 HiLo 图像(94.6% 对比度)。在对传统 HiLo 进行定量分析时,SI 图案的周期相同,我们计算了每对 HiLo-Ground Truth 图像之间的 SSIM 指数。十字型 MLA HiLo 的表现(SSIM = 0.9554)略好于传统 HiLo(SSIM = 0.9396)。然而,在使用六边形 MLA 时,最终 HiLo 图像中出现了明显的伪影(SSIM = 0.9054)。圆柱型 MLA HiLo 结果(SSIM = 0.9366)与传统 HiLo 相似。据我们所知,这是第一项关于基于 MLA 的 HiLo 显微镜的数值研究。这项研究可使使用 MLA 和非相干光源来配置低成本 HiLo 显微镜的研究人员受益匪浅。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optimizing microlens arrays for incoherent HiLo microscopy

HiLo microscopy is a powerful, low-cost, and easily configurable technique for acquiring high-contrast optically-sectioned images. However, traditional HiLo microscopes are based on coherent light sources with diffusive glass plates or incoherent light sources with digital mirror devices (DMD) and spatial light modulators (SLM), which are more expensive. Here, we propose a new low-cost HiLo microscopy technique using MLAs and incoherent LED light sources. We simulated structured illumination (SI) patterns and HiLo image generation. To observe how MLAs affect HiLo images, we used three common MLAs with specific microlens pitch and numerical aperture (NA) to generate periodic illumination patterns. Our simulations concluded that the MLA's NA does not significantly affect HiLo images, and a larger lens pitch can bring a higher image contrast. However, there is an optimized lens pitch. If the lens pitch is equal to or higher than 140 μm, artifacts are observed in HiLo images. Based on our simulations, employing the cross-type MLA with a 0.01NA and a period of 120 μm yields the optimal HiLo image (94.6 % contrast). In our quantitative analysis with the traditional HiLo, where SI patterns were set with the same period, we calculated the SSIM index between each HiLo-Ground Truth image pair. The cross-type MLA HiLo performed slightly better (SSIM = 0.9554) than the traditional HiLo (SSIM = 0.9396). However, when using the hexagon-type MLA, artifacts were evident in the final HiLo image (SSIM = 0.9054). The cylinder-type MLA HiLo result (SSIM = 0.9366) is similar to the traditional HiLo. To our knowledge, this is the first numerical study about MLA-based HiLo microscopy. This study can benefit researchers using MLAs and incoherent light sources to configure their low-cost HiLo microscopes.

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来源期刊
Results in Optics
Results in Optics Physics and Astronomy-Atomic and Molecular Physics, and Optics
CiteScore
2.50
自引率
0.00%
发文量
115
审稿时长
71 days
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