Wide-field (9 × 12 mm) cube scans consisting of 256 B-scans, each with 512 A-scans, were obtained with ssOCT (DRI-OCT; Topcon, Inc., Tokyo, Japan). These scans were used to create maps of RNFL thickness, as well as en face projection images based on reflectance intensity. The latter was generated using special purpose software (ATL 3D-Suite; Fortune B, et al. IOVS 2014;55:ARVO E-Abstract 2644), which is capable of producing en face images in a variety of analysis modes. Slabs through the volume can be defined on the basis of either one or two segmented boundaries. In the first case, a slab can have a fixed thickness, and its axial depth can be defined relative to a reference plane based on a single specific boundary, such as 20 pixels starting at the V/ILM boundary. Alternatively, a slab can be defined by two segmented boundaries such as from the V/ILM to the proximal RNFL boundary. In the latter case, the slab is not constrained to uniform thickness. The axial information at each pixel of the slab can be projected to form the en face image as either the summed voxel projection (SVP), the average voxel projection (AVP), or the maximum intensity projection (MIP). The SVP and MIP images require some form of mapping the intensity values to image space (γ function) that can vary from eye to eye or day to day, whereas the γ function can be fixed across all eyes and scans for AVP images. Therefore, in this study, we obtained AVP en face images for the RNFL and for slabs with a fixed thickness of 52 μm (20 voxels) that were referenced to the V/ILM boundary. The slab thickness of 52 μm was chosen to be small enough to be affected by local differences in reflectance intensity but large enough to benefit from increased signal to noise from averaging over a greater number of voxels. Note that a thickness of 52 μm is larger than the minimum RNFL thickness seen in patients, which is 20 to 30 μm in regions of deep glaucomatous defects. Thus, in regions with a RNFL thickness of less than 52 μm, the slab will include the retinal ganglion cell (RGC) layer and inner plexiform layer, which are hypo-reflective relative to the RNFL. That is, the 52-μm slab incorporates information about both the thickness and reflectance of the RNFL of local regions.
Figure 2 shows images for AVP RNFL (
Figs. 2A, 2C) and the AVP 52-μm slab (
Figs. 2B, 2D) for the eye whose data are shown in
Figure 1. The images on the left were created using the V/ILM and the proximal RNFL boundaries determined by the OCT machines automated algorithm, whereas those on the right were derived after these boundaries were manually corrected. Notice that the appearance of the images for the corrected and uncorrected boundaries was very similar for the AVP 52-μm slab, but markedly difference for the AVP RNFL. This is due to the fact that the automated algorithm is more reliable for the V/ILM boundary than it is for the proximal RNFL boundary.
15,16 For all eyes studied, the details seen on the corrected versions of both the RNFL and 52-μm slab images were similar. Thus, in the interest of making en face imaging clinically useful, the uncorrected AVP 52-μm slab images are used throughout the paper. Except for
Figure 7D, all images are shown in retinal view.