高分辨率光学相干层析成像的角对角和马刺对马刺距离分析。

Eye and vision (London, England) Pub Date : 2020-08-16 eCollection Date: 2020-01-01 DOI:10.1186/s40662-020-00208-0
Robert Montés-Micó, Pedro Tañá-Rivero, Salvador Aguilar-Córcoles, María Ruiz-Santos, María Dolores Rodríguez-Carrillo, Ramón Ruiz-Mesa
{"title":"高分辨率光学相干层析成像的角对角和马刺对马刺距离分析。","authors":"Robert Montés-Micó,&nbsp;Pedro Tañá-Rivero,&nbsp;Salvador Aguilar-Córcoles,&nbsp;María Ruiz-Santos,&nbsp;María Dolores Rodríguez-Carrillo,&nbsp;Ramón Ruiz-Mesa","doi":"10.1186/s40662-020-00208-0","DOIUrl":null,"url":null,"abstract":"<p><strong>Background: </strong>To measure angle-to-angle (ATA) and spur-to-spur (STS) distances along six meridians using high-resolution swept-source optical coherence tomography (SS-OCT) and to compare those values with horizontal white-to-white (WTW) distance.</p><p><strong>Methods: </strong>68 eyes from 68 patients were quantitatively assessed with the Anterion SS-OCT (Heidelberg Engineering, Heidelberg, Germany). ATA and STS distances were measured with the SS-OCT's B-Scan in six cross-sectional images corresponding to the vertical (6-12 o'clock), 1-7 o'clock, 2-8 o'clock, horizontal (3-9 o'clock), 4-10 o'clock and 5-11 o'clock meridians. WTW was measured horizontally with the device's infrared camera. A Pearson correlation analysis was carried out to compare ATA and STS distances with WTW.</p><p><strong>Results: </strong>The largest values were found for the vertical meridian and the shortest for the 2-8 o'clock meridian, both for ATA and STS distances. No statistically significant differences were found between WTW, ATA and STS along the horizontal meridian (<i>p</i> > 0.1). However, ATA and STS showed statistically significant differences elsewhere, except for the horizontal and the 2-8 o'clock meridians (<i>p</i> > 0.05). Moreover, we found that ATA and STS varied significantly depending on the meridian being assessed, except for ATA at 4-10 versus 3-9 o'clock and for STS at 4-10 versus 3-9 o'clock and at 3-9 versus 2-8 o'clock (<i>p</i> > 0.1). R<sup>2</sup> values ranged from 0.49 to 0.75 for ATA and STS at the different meridians, showing the best correlation at 3-9 o'clock meridian (0.64 and 0.75, respectively) and the worst at 6-12 o'clock meridian (R<sup>2</sup> = 0.49 for both ATA and STS).</p><p><strong>Conclusions: </strong>ATA and STS distances vary radially, thus showing that the anterior chamber is vertically oval. Therefore, it is advisable to measure these two distances along the meridian to be used.</p>","PeriodicalId":520624,"journal":{"name":"Eye and vision (London, England)","volume":" ","pages":"42"},"PeriodicalIF":0.0000,"publicationDate":"2020-08-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1186/s40662-020-00208-0","citationCount":"12","resultStr":"{\"title\":\"Angle-to-angle and spur-to-spur distance analysis with high-resolution optical coherence tomography.\",\"authors\":\"Robert Montés-Micó,&nbsp;Pedro Tañá-Rivero,&nbsp;Salvador Aguilar-Córcoles,&nbsp;María Ruiz-Santos,&nbsp;María Dolores Rodríguez-Carrillo,&nbsp;Ramón Ruiz-Mesa\",\"doi\":\"10.1186/s40662-020-00208-0\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p><strong>Background: </strong>To measure angle-to-angle (ATA) and spur-to-spur (STS) distances along six meridians using high-resolution swept-source optical coherence tomography (SS-OCT) and to compare those values with horizontal white-to-white (WTW) distance.</p><p><strong>Methods: </strong>68 eyes from 68 patients were quantitatively assessed with the Anterion SS-OCT (Heidelberg Engineering, Heidelberg, Germany). ATA and STS distances were measured with the SS-OCT's B-Scan in six cross-sectional images corresponding to the vertical (6-12 o'clock), 1-7 o'clock, 2-8 o'clock, horizontal (3-9 o'clock), 4-10 o'clock and 5-11 o'clock meridians. WTW was measured horizontally with the device's infrared camera. A Pearson correlation analysis was carried out to compare ATA and STS distances with WTW.</p><p><strong>Results: </strong>The largest values were found for the vertical meridian and the shortest for the 2-8 o'clock meridian, both for ATA and STS distances. No statistically significant differences were found between WTW, ATA and STS along the horizontal meridian (<i>p</i> > 0.1). However, ATA and STS showed statistically significant differences elsewhere, except for the horizontal and the 2-8 o'clock meridians (<i>p</i> > 0.05). Moreover, we found that ATA and STS varied significantly depending on the meridian being assessed, except for ATA at 4-10 versus 3-9 o'clock and for STS at 4-10 versus 3-9 o'clock and at 3-9 versus 2-8 o'clock (<i>p</i> > 0.1). R<sup>2</sup> values ranged from 0.49 to 0.75 for ATA and STS at the different meridians, showing the best correlation at 3-9 o'clock meridian (0.64 and 0.75, respectively) and the worst at 6-12 o'clock meridian (R<sup>2</sup> = 0.49 for both ATA and STS).</p><p><strong>Conclusions: </strong>ATA and STS distances vary radially, thus showing that the anterior chamber is vertically oval. Therefore, it is advisable to measure these two distances along the meridian to be used.</p>\",\"PeriodicalId\":520624,\"journal\":{\"name\":\"Eye and vision (London, England)\",\"volume\":\" \",\"pages\":\"42\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-08-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1186/s40662-020-00208-0\",\"citationCount\":\"12\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Eye and vision (London, England)\",\"FirstCategoryId\":\"3\",\"ListUrlMain\":\"https://doi.org/10.1186/s40662-020-00208-0\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"2020/1/1 0:00:00\",\"PubModel\":\"eCollection\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Eye and vision (London, England)","FirstCategoryId":"3","ListUrlMain":"https://doi.org/10.1186/s40662-020-00208-0","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2020/1/1 0:00:00","PubModel":"eCollection","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 12

摘要

背景:利用高分辨率扫描源光学相干断层扫描(SS-OCT)测量沿六条子午线的角对角(ATA)和马刺对马刺(STS)距离,并将这些值与水平白对白(WTW)距离进行比较。方法:采用Anterion SS-OCT (Heidelberg Engineering, Heidelberg, Germany)对68例患者的68只眼进行定量评估。采用SS-OCT B-Scan在垂直(6-12点钟)、1-7点钟、2-8点钟、水平(3-9点钟)、4-10点钟和5-11点钟子午线对应的6张横断面图像上测量ATA和STS距离。WTW是用该设备的红外摄像机水平测量的。采用Pearson相关分析比较ATA和STS与WTW的距离。结果:直行子午线与横行子午线距离最大,2-8点钟子午线最短。WTW、ATA和STS沿水平子午线的差异无统计学意义(p > 0.1)。ATA与STS除水平经、2 ~ 8点钟经外,其他部位差异均有统计学意义(p > 0.05)。此外,我们发现ATA和STS根据被评估的子午线有显著差异,除了ATA在4-10与3-9点钟位置,STS在4-10与3-9点钟位置,3-9与2-8点钟位置(p > 0.1)。ATA和STS在不同经络上的R2值为0.49 ~ 0.75,其中3-9点钟经络的相关性最好(分别为0.64和0.75),6-12点钟经络的相关性最差(R2均为0.49)。结论:ATA和STS距离呈放射状变化,表明前房呈垂直椭圆形。因此,沿着子午线测量这两个距离是可取的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Angle-to-angle and spur-to-spur distance analysis with high-resolution optical coherence tomography.

Angle-to-angle and spur-to-spur distance analysis with high-resolution optical coherence tomography.

Angle-to-angle and spur-to-spur distance analysis with high-resolution optical coherence tomography.

Angle-to-angle and spur-to-spur distance analysis with high-resolution optical coherence tomography.

Background: To measure angle-to-angle (ATA) and spur-to-spur (STS) distances along six meridians using high-resolution swept-source optical coherence tomography (SS-OCT) and to compare those values with horizontal white-to-white (WTW) distance.

Methods: 68 eyes from 68 patients were quantitatively assessed with the Anterion SS-OCT (Heidelberg Engineering, Heidelberg, Germany). ATA and STS distances were measured with the SS-OCT's B-Scan in six cross-sectional images corresponding to the vertical (6-12 o'clock), 1-7 o'clock, 2-8 o'clock, horizontal (3-9 o'clock), 4-10 o'clock and 5-11 o'clock meridians. WTW was measured horizontally with the device's infrared camera. A Pearson correlation analysis was carried out to compare ATA and STS distances with WTW.

Results: The largest values were found for the vertical meridian and the shortest for the 2-8 o'clock meridian, both for ATA and STS distances. No statistically significant differences were found between WTW, ATA and STS along the horizontal meridian (p > 0.1). However, ATA and STS showed statistically significant differences elsewhere, except for the horizontal and the 2-8 o'clock meridians (p > 0.05). Moreover, we found that ATA and STS varied significantly depending on the meridian being assessed, except for ATA at 4-10 versus 3-9 o'clock and for STS at 4-10 versus 3-9 o'clock and at 3-9 versus 2-8 o'clock (p > 0.1). R2 values ranged from 0.49 to 0.75 for ATA and STS at the different meridians, showing the best correlation at 3-9 o'clock meridian (0.64 and 0.75, respectively) and the worst at 6-12 o'clock meridian (R2 = 0.49 for both ATA and STS).

Conclusions: ATA and STS distances vary radially, thus showing that the anterior chamber is vertically oval. Therefore, it is advisable to measure these two distances along the meridian to be used.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信