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Purpose: To investigate the impact of corneal higher-order aberrations (HOAs) on predicted corrected distance visual acuity (CDVA) in patients with keratoconus at varying simulated pupil apertures.
Setting: Ophthalmology Clinics, Medical University of South Carolina, Charleston, South Carolina.
Design: Retrospective chart review study.
Methods: 56 eyes with keratoconus were examined using Scheimpflug tomography during routine examinations before medical intervention. The severity of keratoconus was graded using the Amsler-Krumeich classification. Zernike analysis was used to obtain corneal aberrations using simulated pupil diameters of 6 mm, 4 mm, and 2 mm. These data were extrapolated to obtain the total root mean square HOAs for a 1.6 mm simulated pupil to evaluate the potential effect of a small aperture intraocular lens (IOL). Correlation analysis was used to study the impact and relative contributions of HOAs on CDVA. Convolution of HOAs from OPD-Scan III provided a clinical method to predict CDVA with different simulated pupil sizes in corneas with irregular astigmatism.
Results: There were statistically significant positive correlations between photopic CDVA and the magnitude of total and individual (coma, spherical aberration, and trefoil) HOAs in this cohort of keratoconus participants. A keratoconus case with the small aperture IOL confirms the improvement in vision due to the pinhole effect.
Conclusions: The small aperture IOL is expected to markedly reduce aberrations in patients with keratoconus up to Amsler-Krumeich class 4 severity to levels consistent with the levels seen in healthy patients. Convolution of corneal HOAs with the Early Treatment Diabetic Retinopathy Study chart provides a useful simulation of the impact of pinhole optics in aberrated eyes.
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http://dx.doi.org/10.1097/j.jcrs.0000000000001480 | DOI Listing |
Small Methods
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Green and Sustainable Materials R&D Department, Korea Institute of Industrial Technology (KITECH), Cheonan, Chungcheongnam-do, 31056, Republic of Korea.
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View Article and Find Full Text PDFRev Sci Instrum
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Department of Physics, Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan.
We present the design methodology and characterization of a superconducting magnetic bearing (SMB) system for the polarization modulator in the small aperture telescope-low-frequency (SAT-LF), one of the SATs of the Simons Observatory (SO) that is sensitive at 30/40 GHz. SO is a cosmic microwave background (CMB) polarization experiment, with SATs targeting the search for primordial parity-odd polarization anisotropies at degree scales. Each SAT uses a cryogenic, rotating half-wave plate (HWP) as a polarization modulator to reduce atmospheric 1/f noise and instrumental systematics.
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