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Acrysof SN60WF人工晶状体与Eternity Natural Uni NW-60人工晶状体之间的闪光形成及其对前向光散射影响的比较。

Comparison of glistenings formation and their effect on forward light scatter between the Acrysof SN60WF and Eternity Natural Uni NW-60 intraocular lenses.

作者信息

Philippaki Eva, O'Brart David P, Hull Chistopher C

机构信息

Physics, King's College London, London, UK.

Guy's and Saint Thomas' NHS Foundation Trust, London, UK.

出版信息

BMJ Open Ophthalmol. 2020 Feb 12;5(1):e000399. doi: 10.1136/bmjophth-2019-000399. eCollection 2020.

DOI:10.1136/bmjophth-2019-000399
PMID:32154371
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7044831/
Abstract

AIMS

To compare the characteristics of glistenings and forward light scatter between the Alcon Acrysof SN60WF and Santen Eternity Natural Uni NW-60 intraocular lenses (IOLs).

METHODS

Five Acrysof SN60WF and five Eternity Natural Uni NW-60 IOLs were studied. All IOLs were single piece blue blockers with the same dioptric power (20D) and optic diameter (6.0 mm). Glistenings were induced by a thermal accelerated ageing process. Glistenings were objectively quantified using bespoke image processing software. The angular distribution of forward light scatter was measured using an optical bench system and the straylight parameter calculated from the light scatter function.

RESULTS

The median increase in the number of glistenings was 15 and 525 for the Eternity and Acrysof IOLs, respectively, which was statistically significantly different (p=0.012). Median glistenings diameter was 23.8 μm (Acrysof) and 32.8 μm (Eternity). Four (80%) of the Acrysof lenses had straylight values higher than a 20-year-old CIE standard glare observer and in two cases the straylight exceeded that of the 70-year-old CIE standard glare observer. None of the Eternity lenses had straylight values that exceeded the value for the 20-year-old CIE standard glare observer.

CONCLUSIONS

The Eternity Natural Uni NW-60 IOLs resisted the induction of glistenings more than the Acrysof SN60WF IOLs. Although the Acrysof IOLs developed smaller glistenings than the Eternity IOLs, there were sufficient numbers to produce a higher straylight parameter.

摘要

目的

比较爱尔康Acrysof SN60WF和参天Eternity Natural Uni NW - 60人工晶状体(IOL)的闪光和前向光散射特性。

方法

研究了5枚Acrysof SN60WF和5枚Eternity Natural Uni NW - 60 IOL。所有IOL均为单片蓝色阻断型,具有相同的屈光力(20D)和光学直径(6.0毫米)。通过热加速老化过程诱导产生闪光。使用定制的图像处理软件对闪光进行客观量化。使用光具座系统测量前向光散射的角度分布,并根据光散射函数计算杂散光参数。

结果

Eternity和Acrysof IOL的闪光数量中位数增加分别为15和525,差异具有统计学意义(p = 0.012)。闪光直径中位数为23.8μm(Acrysof)和32.8μm(Eternity)。4枚(80%)Acrysof晶状体的杂散光值高于20岁的CIE标准眩光观察者,在2例中杂散光超过了70岁的CIE标准眩光观察者。Eternity晶状体的杂散光值均未超过20岁的CIE标准眩光观察者的值。

结论

Eternity Natural Uni NW - 60 IOL比Acrysof SN60WF IOL更能抵抗闪光的诱导。尽管Acrysof IOL产生的闪光比Eternity IOL小,但数量足够产生更高的杂散光参数。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/1c5afd6e10e8/bmjophth-2019-000399f05.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/ea06e6d9333f/bmjophth-2019-000399f01.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/16d6ecac1de8/bmjophth-2019-000399f02.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/4801bace1b5b/bmjophth-2019-000399f03.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/8ab68cd220ac/bmjophth-2019-000399f04.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/1c5afd6e10e8/bmjophth-2019-000399f05.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/ea06e6d9333f/bmjophth-2019-000399f01.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/16d6ecac1de8/bmjophth-2019-000399f02.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/4801bace1b5b/bmjophth-2019-000399f03.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/8ab68cd220ac/bmjophth-2019-000399f04.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a336/7044831/1c5afd6e10e8/bmjophth-2019-000399f05.jpg

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