Optical bench testing of IOLs has already been described in earlier works
21,22 and is summarized here for the sake of conciseness. The setup is shown in
Figure 1, where the inset illustrates the LCA affecting the distance and near foci of an exemplary diffractive bifocal lens
1 that uses the base lens curvature and zeroth and first diffraction orders to achieve simultaneous distance and near foci, respectively. The intermediate focus existing in the case of a trifocal IOL has been omitted for the sake of simplicity.
Three R, G, and B light-emitting diodes (LEDs; Thorlabs, Inc., Newton, NJ) with nominal wavelengths of 455 nm (B), 530 nm (G), and 625 nm (R) and full width at half maximum of 18 nm for the B and R LEDs and 33 nm for the G LED were sequentially used to illuminate the setup. A 200-µm pinhole test object was placed at the front focal plane of a collimating lens. The collimated beam illuminated the wet cell where the IOL was inserted. The IOL imaged the pinhole either on separate image planes (as corresponds to multifocal lenses) or on a focal segment (as corresponds to EDOF lenses). A diaphragm placed in front of the wet cell and used as the entrance pupil limited the IOL aperture to a diameter of 3.5 mm throughout the test. Even with such an intermediate pupil (3.5 mm), the impact of the negative spherical aberrations of all tested IOLs on their images was still relatively low. This fact helped us to compute the energy efficiency metric. Additionally, we kept the same pupil size as used in former papers of ours (Refs.
21 and
22) so that further comparisons with lenses of various designs could be done.
Behind the wet cell an infinite corrected microscope mounted on a translation holder focused the aerial image of the pinhole and magnified it onto a monochrome 8-bit charge-coupled device camera (Wells Research and Development, Inc., Lincoln, MA) used for digital image acquisition. The microscope objective (4× Olympus Plan Achromat; Olympus Corp., Tokyo, Japan), suited for high-quality imaging applications, had diffraction-limited performance through the visible spectrum. The microscope and camera moved together along the bench axis to precisely locate the positions of the focal planes for each IOL with a spatial resolution of 1 µm. Axial scanning was stretched to smoothly cover the focal segment of interest—from distance to intermediate and near images—in trifocal and EDOF IOLs. More precisely, through-focus measurements covered an image vergence range of about 7 D (range, +2.0 to –5.0 D) in 0.1-D steps with 0.05-D resolution. To improve the signal-to-noise ratio, each image was eventually the result of averaging eight image frames.
The RGB TF-EE of each IOL was measured.
Figure 2 illustrates the procedure used to calculate the energy efficiency (EE) that was measured in the image space. An edge detection algorithm, Canny edge detector, as implemented by MATLAB (MathWorks, Natick, MA) was first applied to segment the central core from the image of the pinhole at a given image focus plane. In every focus (distance, intermediate, and near), a local maximum EE value (which also involved a peak in the area under the modulation transfer function curve) determined the position of the best focus plane.
Figure 2A shows the pinhole image under G light at the distance focus plane of a lens, which corresponds to an image vergence of 0.0 D. Then, the intensity in the image as a whole was calculated (
Itotal =
Icore +
Ibackground) to obtain the EE metric from the
Icore/Itotal ratio: EE (%) = (
Icore/
Itotal) × 100. The EE metric was easy to compute for the three R, G, and B wavelengths and under experimental conditions approached the so-called light-in-the-bucket metric.
20,35 By definition, the light-in-the-bucket metric represents the diffraction EE of an IOL, as well as the image blur caused by aberrations and scattering, because it quantifies the amount of light in the central core of the point spread function (PSF) relative to that of a monofocal diffraction-limited PSF for the same wavelength and pupil size.
20,35 The implementation of this metric in experimental practice, where the ideal point source is replaced by a pinhole of certain size, has been described and justified in a former work.
21
The procedure was then repeated step by step to axial scan the region of interest (from +2.0 to –5.0 D, in 0.1-D steps with 0.05-D resolution) in trifocal and EDOF IOLs.
The focus powers and their corresponding LCAs were experimentally obtained in all lenses from the maxima of the RGB TF-EE curves. LCA values were computed from the power difference between the B and R EE peaks at each focus plane. For an achromatized lens, for which the B – R power difference is ideally reduced to zero, we also computed the residual chromatic aberration from the maximum power difference between the G EE peak and the R and B ones. The distance power was measured with respect to the distance focus at G illumination (closest to the design wavelength according to the ISO 11979-2:2014). At such a G distance focus plane, the image vergence was set to 0.0 D. Further details can be found elsewhere.
21,22
The following additional metrics are defined here and were included in the analysis for a more complete characterization of the chromatic performance of the lenses: