Gantes-Nuñez Javier, Jaskulski Matt, López-Gil Norberto, Kollbaum Pete S
Indiana University School of Optometry, Bloomington, Indiana, USA.
CiViUM Research Group, Universidad de Murcia, Murcia, Spain.
Ophthalmic Physiol Opt. 2023 May;43(3):388-401. doi: 10.1111/opo.13098. Epub 2023 Feb 4.
To quantify the amount of myopic defocus, contrast modulation and other optical characteristics of two novel spectacle lenses (MiYOSMART by Hoya and Stellest by Essilor) with the inclusion of lenslets in their designs were investigated computationally and experimentally. This paper examined the hypothesis that despite the non-coaxial nature of the optics, image degradation will exist due to the fragmented nature of the base optic when imaging through the lens regions populated by lenslets.
Optical power was evaluated by computing wavefront vergence and curvature from wavefront slope measured with the Optocraft aberrometer within 1.0 and 6.0 mm apertures across MiYOSMART hexagons and Stellest rings. Point-spread functions (PSFs) were computed using physical (wave) optics and geometrical ray optics principles, and compared with experimental measurements using a 4f optical system. Simulated retinal images and modulation transfer functions (MTFs) were computed from PSF-derived optical transfer functions (OTFs).
Mean lenslet power in MiYOSMART was +3.95 ± 0.10 D through the hexagons and +6.00 ± 0.15 D in Stellest in rings 1-5 and decreased by 0.42 D/ring reaching 3.50 D in the final one. Stellest lenslets included up to -0.015 microns of primary spherical aberration. PSFs and retinal images revealed simultaneous contributions of the base optic and lenslets. MTFs showed a decrease in contrast at low (1-10 c/deg) spatial frequencies (SFs) comparable to 0.25 D of defocus, and retention of diminished levels of contrast at higher SFs.
Varying sagittal power and consistent curvature power across the lenslets is an identifying signature of the novel non-coaxial lens design included in both spectacle lenses. Lenslet array structure itself plays a significant role in determining image characteristics. For both lenses, the blur created by the fragmented base optic contributes to the image quality. The reduced MTFs over a wide range of spatial frequencies result in lowered image contrast.
通过计算和实验研究两种新型眼镜镜片(豪雅的MiYOSMART和依视路的Stellest)的近视离焦量、对比度调制及其他光学特性,这两种镜片在设计中均包含微透镜。本文检验了这样一个假设:尽管光学系统是非同轴的,但当通过由微透镜组成的镜片区域成像时,由于基础光学元件的碎片化性质,仍会存在图像退化现象。
通过使用Optocraft像差仪在1.0至6.0毫米孔径范围内测量波前斜率,计算MiYOSMART六边形和Stellest环的波前聚散度和曲率,从而评估光焦度。使用物理(波动)光学和几何光线光学原理计算点扩散函数(PSF),并与使用4f光学系统的实验测量结果进行比较。从PSF导出的光学传递函数(OTF)计算模拟视网膜图像和调制传递函数(MTF)。
MiYOSMART中微透镜的平均光焦度在六边形区域为+3.95±0.10 D,在Stellest的第1至5环中为+6.00±0.15 D,在最后一环中以每环0.42 D的速率下降至3.50 D。Stellest微透镜包含高达-0.015微米的初级球差。PSF和视网膜图像显示了基础光学元件和微透镜的共同作用。MTF显示在低(1-10周/度)空间频率下对比度下降,相当于0.25 D的离焦,并且在较高空间频率下保持降低的对比度水平。
微透镜上变化的矢状光焦度和一致的曲率光焦度是这两种眼镜镜片中新型非同轴镜片设计的识别特征。微透镜阵列结构本身在决定图像特性方面起着重要作用。对于这两种镜片,基础光学元件碎片化产生的模糊会影响图像质量。在很宽的空间频率范围内MTF降低导致图像对比度下降。