Measurements were obtained with a custom-built instrument (Indiana Scanning Aberrometer for Wavefronts,
I SAW, shown schematically in
Figure 1) designed to measure ocular aberrations at 850 nm over a 30° diameter field of view centered on the foveal line-of-sight. The instrument measures aberrations associated with a particular location in the visual field by focusing a spot of light (the “retinal beacon”) on the retinal surface at the corresponding retinal location. Light reflected out of the eye from the retinal beacon is captured by a wavefront sensor for analysis. Due to variations in head size and shape, the full 30° field could not be accessed in all subjects without vignetting of the Shack-Hartmann sensor (Adaptive Optics Associates, Inc., Cambridge, MA) in some visual field locations. By reducing the maximum tested eccentricity to 13.5° it became possible to measure the central 27° diameter field completely in all subjects. Although wavefront aberrations have been reported for eccentricities beyond 13.5° (Jaeken & Artal,
2012; Lundstrom et al.,
2009; Mathur et al.,
2009), in our experience accurate measurements are limited to about 30° of eccentricity if the aberrometer relies on the Shack-Hartmann wavefront sensor for pupillometry (Shen, Clark, Soni, & Thibos,
2010). Defocus measurements were corrected to 552 nm (the centroid of the luminance spectrum of the accommodation target) using the Indiana Eye model of ocular chromatic aberration (Coe, Bradley, & Thibos,
2014; Nam, Rubinstein, & Thibos,
2010; Thibos, Ye, Zhang, & Bradley,
1992). Design principles, technical specifications, and validation results for the basic instrument are available elsewhere (Wei & L. Thibos,
2010). For the current study the instrument's dynamic range was expanded by introducing a pair of relay lenses in a Badal configuration (Goncharov, Nowakowski, Sheehan, & Dainty,
2008) to enable the measurement of eyes over a wide range of refractive states (+8 D to −10 D). The instrument's data acquisition rate (2 visual field locations per second) was sufficient to sample the central visual field in a randomized sequence of 37 locations [eccentricities 0°, 5°, 10°, 13.5° along 12 visual meridians 0° to 360° in 30° steps] in approximately 16 s. Normal blinking was permitted, with subsequent rejection of corrupted data images by quality control procedures. Wavefronts reflected from the eye were descanned by the scanning mirrors and directed into a conventional Shack-Hartmann wavefront sensor, which reported wavefront aberrations in the form of Zernike polynomial coefficients (American National Standards Institute,
2004).