A single trained technician performed AS-OCT imaging using the quad-scan mode, which ensures that images of the anterior segment are captured simultaneously along the four meridians (45, 90, 135, and 180°). Subjects adapted to the dark (0 lux) for at least 5 minutes prior to imaging (
Fig. 1, top) and were imaged again after a brief pause while exposing the fellow eye to bright light (pen light, 1700 Lux;
Fig. 1, bottom). The fellow eye was continuously exposed to the pen light during this phase of image capture process.
We analyzed OCT images using custom semiautomated software (Zhongshan Angle Assessment Program [ZAAP], Guangzhou, China).
21 An experienced observer (CZ) marked the scleral spur in each image and from this the software generated the following parameters (
Fig. 2A): iris cross-sectional area, iris volume, anterior chamber width (ACW), iris curvature, iris thickness (IT750 and IT2000), and lens vault. The iris cross-sectional area was calculated as the cumulative cross-sectional area of the full length (from spur to pupil) of the iris. Iris volume calculations were based on the principles of centroid theorem.
22 In brief, the centroid and its coordinate were identified as an average of all pixel coordinates within the cross-sectional area by the software. The distance from centroid to the AC axis was defined as the radius, and the iris volume was then calculated by rotating the iris cross-sectional area along this radius. The ACW was defined as the horizontal scleral spur-to-spur distance and the lens vault was measured by estimating the perpendicular distance between the anterior pole of the crystalline lens and the horizontal line joining the two scleral spurs (
Fig. 2B). The iris curvature (I-Curv) was estimated by the software by drawing a line from the most peripheral to the most central points of iris pigment epithelium and then a perpendicular line was extended from this line to the iris pigment epithelium at the point of greatest convexity. The IT750 and IT2000 were defined as the iris thickness (IT) measured at 750 and 2000 μm from the scleral spur, respectively. Averages of iris volume and cross-sectional area were obtained from three meridians (45, 135, and 180°) in each condition of illumination. The sum of average iris volume and iris cross-sectional areas from the nasal temporal sectors of the iris were designated as total iris volume and cross-sectional area, respectively, for that eye and that specific illumination condition. The 90° images were not used for analysis due to frequent lid artifacts resulting in poor cross-sectional images along that meridian. Average pupil diameter was measured and calculated using the caliper function of the software from the three meridians used (45, 135, and 180°) for both light and dark conditions. Images obtained in the dark were designated as baseline and averages of ACW, I-Curv, IT750, and lens vault were determined from these images. Changes in total iris volume and cross-sectional area between conditions of light and dark were evaluated in a multivariate model that included diagnostic groups and associated ocular and demographic factors.