One can estimate the theoretical DOF by calculating the range of defocus errors, which degrades the retinal image quality to a certain level of the possible maximum value. This definition has been adopted earlier by Marcos et al. (
1999), who chose an 80% threshold, while a 50% threshold was used by Jansonius and Kooijman (
1998) and Legge et al. (
1987). In this study, we chose the augmented visual Strehl ratio based on the optical transfer function (VSOTF) as the retinal image quality predictor to estimate the matching threshold based on the subjectively measured DOF.
The VSOTF is currently considered one of the best descriptors of visual performance that can be directly derived from the wavefront aberrations data (Marsack, Thibos, & Applegate,
2004) and is strongly correlated with the subjective visual acuity (Cheng, Bradley, & Thibos,
2004). We have used its augmented version (Iskander,
2006), i.e.,
where
OTFDL(
fx,
fy) denotes the diffraction limited optical transfer function,
CSFN(
fx,
fy) is the neural contrast sensitivity function, and (
fx,
fy) are the spatial frequency coordinates. Here the VSOTF was based on calculated optical transfer function across all spatial frequencies up to 60 cycles per degree (Iskander,
2006).
To estimate DOF from an image quality metric, a through-focus calculation is required. A dedicated simulation program was written from first principles in Matlab (The MathWorks, Natick, MA) to calculate the through-focus VSOTF in the presence of the subject's original higher order aberrations (HOAs). The flow chart of the computer simulation program is shown in
Figure 2.
In the first step, wavefront data, consisting of a set of Zernike coefficients up to and including the 8th radial order, are imported. Since the wavefront data was acquired for the subject's dilated pupils always larger than 5 mm, for consistency, in step 2, the original Zernike coefficients were resampled to a specific pupil diameter of either 5 mm or 3.5 mm using the method of Schwiegerling (
2002).
Since the subject's sphero-cylindrical error was corrected during the subjective DOF measurements, only the effect of HOAs on VSOTF is considered in the simulation. The estimates of sphero-cylinder need to be first removed from the wavefront. One can achieve that by simply setting the first six Zernike coefficients to zero. However, it has been shown that the Maloney's best sphero-cylinder (S/C) calculated in the refractive power domain has the best correlation to the subjective sphero-cylindrical refractive error of the eye (Iskander, Davis, Collins, & Franklin,
2007). Hence, a transformation from the wavefront domain to the refractive power domain is performed. In step 3, the refractive power distribution across the pupil,
F(
r, θ), is calculated from the resampled wavefront
W(
r, θ) using the method of the refractive Zernike power polynomials (Iskander, Davis, Collins, & Franklin,
2007):
where
Z{·} denotes the wavefront to refractive power transformation.
Following that, in step 4, the best S/C is estimated using the method of Maloney, Bogan, and Waring (
1993) and subtracted from the previously obtained refractive power. This leads to the new refractive power, given by
where
FZer and
FSC is the refractive power calculated from the subject's original wavefront and the estimated best S/C, respectively. To simulate through focus, in the through-focus loop, a desired level of defocus is added to the refractive power from step 4. In step 5, an inverse transformation from the refractive power domain to the wavefront domain is performed (Iskander, Davis, & Collins,
2007):
which is then used, in step 6, to calculate the VSOTF. From the wavefront
Wout(
r, θ) with a new defocus value, the corresponding point spread function and the optical transfer function (OTF) is calculated using fast Fourier transforms (Artal,
1990; Iskander, Collins, Davis, & Carney,
2001). The through-focus VSOTF is obtained in step 7. The calculation was repeated in a total of 49 steps corresponding to a defocus level ranging from −3 D to +3 D in 0.125-D intervals.
An example of how the matching threshold value is estimated for data acquired from averaged wavefront measurements of a subject in a 5-mm pupil is shown in
Figure 3. After obtaining the through-focus VSOTF of the subject from wavefront data, an iterative calculation was performed, reducing the threshold level from 99% of the maximum achievable VSOTF value, until the effective range of defocus error produced by
D 2 −
D 1 gives the closest match to the subjectively measured DOF. This threshold value was taken as the matching threshold to estimate the DOF for this subject. The same procedure was performed for measurements of each individual subject.