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, Pedro Tañá-Rivero, Salvador Aguilar-Córcoles, María Ruiz-Santos, María Dolores Rodríguez-Carrillo, 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, Pedro Tañá-Rivero, Salvador Aguilar-Córcoles, María Ruiz-Santos, María Dolores Rodríguez-Carrillo, 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}
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.