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1 From the Instituto de Optica "Daza de Valdés," Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain; and the 2 Instituto de Oftalmobiología Aplicada, Universidad de Valladolid, Spain.
| Abstract |
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METHODS. Total and corneal aberrations were measured in a group of 14 eyes (preoperative myopia ranging from -2.5 to -13 D) before and after LASIK surgery. Total aberrations were measured using a laser ray-tracing technique. Corneal aberrations were obtained from corneal elevation maps measured using a corneal system and custom software. Corneal and total wave aberrations were described as Zernike polynomial expansions. Root-mean-square (RMS) wavefront error was used as a global optical quality metric.
RESULTS. Total and corneal aberrations (third-order and higher) showed a statistically significant increase after LASIK myopia surgery, by a factor of 1.92 (total) and 3.72 (corneal), on average. This increase was more pronounced in patients with the highest preoperative myopia. There is a good correlation (r = 0.97, P < 0.0001) between the aberrations induced in the entire optical system and those induced in the anterior corneal surface. However, the anterior corneal spherical aberration increased more than the total spherical aberration, suggesting also a change in the spherical aberration of the posterior corneal surface. Pupil centration and internal optical aberrations, which are not accounted for in corneal topography, play an important role in evaluating individual surgical outcomes.
CONCLUSIONS. Because LASIK surgery induces changes in the anterior corneal surface, most changes in the total aberration pattern can be attributed to changes in the anterior corneal aberrations. However, because of individual interactions of the aberrations in the ocular components, a combination of corneal and total aberration measurements is critical to understanding individual outcomes, and by extension, to designing custom ablation algorithms. This comparison also reveals changes in the internal aberrations, consistent with the posterior corneal changes reported using scanning slit corneal topography.
| Introduction |
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Recently, the implementation of techniques to precisely measure the optical wave aberration pattern9 10 11 12 13 14 15 16 before and after refractive surgery has generated significant excitement among specialists in refractive surgery. First, the measurement of optical defects (aberrations) after refractive surgery has revealed that, although conventional refractive errors (i.e., myopia or astigmatism) are reduced or canceled, higher order aberrations (uncorrectable by conventional means) are generally induced.17 18 19 20 Second, along with other technical developments (e.g., scanning small-spot lasers, eye trackers), the precise measurement of ocular wave aberrations has opened the potential for improved refractive surgery that is customized for each patient and intended to cancel both low- and high-order aberrations in the eye.21 22 23 24 Two approaches are currently being pursued, both to evaluate and to guide ablation procedures: wavefront aberrations (aberrations of the entire optical system)18 21 and corneal topography25 26 27 (alternatively, aberrations of the anterior corneal surface). Analysis of the total aberrations of the eye provides the most direct and complete measurement of retinal image quality and therefore can be directly related to visual performance. Previous studies show high correlations between corneal aberrations (wavefront variance) and visual performance (area under contrast sensitivity function).28
We have shown that most of the decrease in contrast sensitivity found after LASIK can be explained by a decrease in the modulation-transfer function computed directly from the wave aberration.29 However, because in refractive surgery changes are induced only in the cornea, the question arises whether corneal topography would be sufficient to fully predict visual outcomes.7 In this article, we present corneal and total aberrations in the same eyes before and after LASIK for myopia. We show that the combination of these two pieces of information is important in understanding individual surgical outcomes (which becomes critical in customizing ablation algorithms). It also provides insights into the biomechanical response of the cornea (both the anterior and posterior surfaces) to laser refractive surgery.
| Methods |
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LASIK Surgery
Standard LASIK surgery was conducted using a narrow-beam,
flying-spot excimer laser (Chiron Technolas 217-C equipped with the
PlanoScan program; Bausch & Lomb Surgical, Madrid Spain). This
laser has an emission wavelength of 193 nm, a fixed pulse repetition
rate of 50 Hz, and a radiance exposure of 400 mJ. The procedure was
assisted by an eye tracker. The flap diameter (performed with a
Hansatome microkeratome; Bausch & Lomb España, SA, Madrid Spain)
was 8.5 mm, and the intended depth was 180 µm. Photoablation was
applied to a 6-mm optical zone, with a transition zone of 9 mm. The
LASIK procedures were conducted at the Instituto de
Oftalmobiología Aplicada, Universidad de Valladolid, Spain.
Total Aberrations Using LRT
Total wave aberrations were measured using laser ray tracing
(LRT), developed at the Instituto de Optica in Madrid,
Spain.12
The principles30
31
and, in
particular, its use as an evaluation tool in LASIK surgery for myopia,
have been described in detail elsewhere.18
In this
technique, a scanning system scans a narrow laser beam (543 nm) across
the pupil. Simultaneously, a high-resolution charged-coupled device
(CCD) camera captures the retinal spot images corresponding to each
entry pupil location. Figure 1A
shows a particular series of images after surgery in a LASIK-treated
eye. The positions of the centroids of the set of retinal images form a
spot diagram (Fig. 1B)
. The deviations of each centroid from the
principal ray are proportional to the local slopes of the wave
aberration. Each run consists of 37 rays, sampling a 6.5-mm pupil in
1-mm steps in a hexagonal pattern, and lasts 4 seconds. Each
measurement is repeated five times.
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, spherical
aberration) or the RMS for third-order terms and higher, i.e.,
excluding piston
(
), tilts
(
and
Z
), defocus
(Z
) and
astigmatism (Z
and Z
), and
for isolated Z terms. In these group of patients, Zernike
coefficient SD (averaged across terms) ranged from 0.026 to 0.170 µm
(mean, 0.069 ± 0.037 µm [SD]).
Corneal Aberrations from Corneal Topography
Corneal height numerical data were obtained with a corneal
topography system (Atlas Mastervue; Humphrey Instruments-Zeiss, San
Leandro, CA). These data were processed using custom software (Matlab;
Mathworks, Natik, MA) and exported to an optical design program (Zemax
ver. 9; Focus Software, Tucson, AZ), which performed a ray-tracing
simulation to compute corneal aberrations from corneal topography
data.32
33
34
35
This technique has been validated in
recent studies of keratoconus and aphakia.36
Both
the corneal surface and the corneal aberration pattern (at the plane of
best focus) were described by a Zernike polynomial expansion. We
checked that a seventh-order polynomial expansion represented a good
description of the surface: the RMS error of the fitting was 0.43 ± 0.11 before surgery and 0.53 ± 0.11 after surgery (average
across the eyes of this study). This error is lower than the accuracy
of the corneal topography devices, which can measure surfaces to an RMS
error of 3.7 ± 0.7 µm.37
Figure 1C shows a corneal elevation map (10-mm diameter, centered on the corneal reflex) for the same eye as in Figure 1A . To show the irregularities, we subtracted the first six terms of a Zernike polynomial fit to the height data from the raw height data.34 Ray aberrations were obtained by virtual ray tracing, sampling 64 x 64 points of the corneal surface (in a rectangular grid). Figure 1D shows a spot diagram corresponding to a subset of 91 rays, through a 6.5-mm corneal region centered at -0.6 to +0.6 mm from the corneal reflex. The indices of refraction were taken as that of the air and the aqueous humor (1.3391). For this analysis, the corneal index of refraction was not considered. Wavelength was set to 543 nm (as in the LRT measurements). Unlike the LRT measurements (for which the reference was the pupil center), corneal topography typically uses the corneal reflex (location of the first Purkinje image when the subject fixates foveally) for alignment. Proper alignment of corneal and total aberration is necessary for direct comparison.
We developed custom software to locate the colinear pupil
position.36
Corneal aberrations were computed over a large
pupil diameter (10 mm) and recomputed over a 6.51-mm pupil (matching
the pupil size of total aberration measurements), moving the center
over a ±1-mm grid, in 0.1-mm steps. A difference
total-corneal map was computed for each pupil location. These maps were
smooth and in all cases showed a clear, single minimumtypically,
slightly decentered from the corneal reflex. Despite the underlying
assumptions, independent observations36
in control
subjects showed that this procedure identifies well the pupil center
(inaccessible otherwise from the corneal topography images). Apart from
the decentration between the corneal reflex and pupil center, the
keratometric axis is tilted with respect to the line of sight. This
angle can be computed by measuring the distance between the corneal
intersect of the keratometric axis and corneal sighting center (not
available in our patients) and using the fixation point distance.
Mandell38
reported an average difference of 0.38 ±
0.10 mm between the corneal intersect of the keratometric axis and the
corneal sighting center across 20 normal eyes. Assuming similar values
in our group of eyes and for the 148.3-mm fixation point distance in
our videokeratoscope, the neglected corneal tilt is approximately
0.15°. For a typical cornea (eye 10) we found that, considering this
tilt, RMS changes by only 2.7% before surgery and 0.68% after surgery
for third-order Z terms and by 0.46% before surgery and
0.15% after surgery for spherical aberration
(Z
).
In this particular experiment, we obtained only one corneal map per eye and per session. Experiments in one control eye (RMS = 0.59 µm, for third- and higher order terms) showed a Zernike coefficient SD of 0.016 (averaged across terms). Experimental centration errors (SDs) were 0.08 mm for the horizontal coordinate and 0.08 mm for the vertical coordinate.
| Results |
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Figure 4
shows the change of the fourth-order spherical aberration coefficient
(
), both total
(Fig. 4A)
and corneal (Fig. 4B)
. Sign and normalization follow the
convention suggested by the Optical Society of America Standardization
Committee.41
The preoperative total spherical aberration
coefficient was close to zero in most eyes (significantly positive in
seven eyes and significantly negative in three eyes). Preoperative
corneal spherical aberration was positive in all eyes, except for one
that was not significantly different from zero. Total spherical
aberration increased significantly with LASIK in all eyes and corneal
spherical aberration in all but one eye. The most dramatic increase
occurred in patients with the highest preoperative myopia, both for
total18
and corneal aberrations.33
42
Total
spherical aberration
coefficient
for the pre- minus postoperative difference ranged from 0.22 to 1.64
µm (0.63 µm, on average), and for the cornea the differences ranged
from -0.01 to 1.72 µm (0.74 µm on average). The increase of
spherical aberration seems to be more pronounced for corneal than for
total aberrations.
|
also). There
was a very good correlation between corneal and total aberrations
(third-order and higher) after LASIK (r = 0.97,
P < 0.0001; slope = 1.01; Fig. 5A
). The corneal
spherical aberration after LASIK was also well correlated to the total
spherical aberration after LASIK (r = 0.91,
P < 0.0001; slope = 1.22; Fig. 5B
). However, that
the slope is significantly higher than 1 suggests that a larger
spherical aberration is induced in the anterior corneal surface than in
the entire eye. A higher slope in the post-LASIK corneal versus total
aberration was found for the RMS of the spherical aberration, the
spherical aberration coefficient
(
), and the RMS
of fourth-order Z terms, but not for third-order aberrations
or all high-order aberrations (third-order and higher).
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Figure 6
shows the spherical aberration coefficient
after LASIK
as a function of preoperative spherical refractive error, for corneal,
total, and internal aberrations. The internal aberration coefficients
were computed as the total minus the corneal coefficients. There was a
statistically significant increase of the absolute amount of
postoperative spherical aberration for total (r = 0.80,
P = 0.0003), corneal (r = 0.92,
P < 0.0001), and internal (r = 0.73,
P = 0.0024) aberrations with preoperative refractive
error. However, the total spherical aberration increased less than the
spherical aberration in the anterior corneal surface, because of the
spherical aberration of negative sign induced on the posterior corneal
surface. The same analysis for post-LASIK third-order aberrations shows
no statistically significant difference between corneal and total
aberrations. Therefore, third-order aberrations do not seem to be
induced in the posterior corneal surface.
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| Discussion |
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Role of Pupil Centration
Several studies have shown the impact of refractive surgery for
myopia (radial keratotomy [RK] and photorefractive keratectomy
[PRK]) on corneal aberrations.25
33
43
As in the present
analysis, those studies computed the corneal aberration pattern by
measuring corneal elevation maps using commercial corneal
videokeratoscopes. In these devices, centration is typically achieved
by aligning a set of concentric rings to the corneal reflex of the
fixation light. Corneal aberrations are then typically referred to the
corneal reflex rather than the pupil center. Our processing algorithms
align the corneal aberration pattern with the total aberration pattern,
which is referred to the pupil center. The position of the pupil is
important for a correct estimation of retinal image
quality44
and should be taken into account when predicting
visual performance from corneal aberration data. According to our
computations, corneal aberration data (third-order and higher) changed
by 10% when the pupil position was taken into account. Although, as
expected, spherical aberration did not change significantly by
recentration (3% on average), third-order aberrations changed by 22%.
Figure 7 shows the corneal aberration pattern for the same post-LASIK eye (eye
10), centered at the corneal reflex (Fig. 7
, right; as directly
processed from the corneal topographer raw data) and at the pupil
center (left). First- and second-order Z terms (which also
changed with decentration) are excluded in each map. Although direct
corneal data show no coma, when the actual pupil position is taken into
account, we observed that coma is predominant along with spherical
aberration.
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Furthermore, it is not uncommon (35%) that the amount of negative
internal spherical aberration (likely from the crystalline
lens46
47
) exceeds the amount of positive spherical
aberration of the anterior corneal surface. Figure 8
illustrates one of these cases (eye 6), with a corneal preoperative
spherical aberration
(
) of 0.38 µm
and internal preoperative aberration of -0.48 µm. The upper row
shows the measured total and corneal and the computed internal
aberration patterns. The negative internal aberration dominates the
central area total aberration pattern. After LASIK (lower row),
positive spherical aberration is induced on the anterior corneal
surface, which cancels (actually overcompensates) the preoperative
negative spherical aberration of the internal optics. For this reason,
the post-LASIK total aberration pattern for this eye is much better
than predicted from corneal aberrations alone. Unlike other subjects
with similar preoperative myopia and similar corneal topography after
LASIK, this subject did not show any loss of contrast sensitivity
(actually improved at two spatial frequencies).29
|
LASIK-Induced Posterior Corneal Aberrations and Biomechanical
Response
Comparison of post-LASIK corneal and total aberrations revealed an
increase in the amount of negative internal spherical aberration, which
tended to slightly attenuate the impact of the positive spherical
aberration induced in the anterior corneal surface (Fig. 6)
. The effect
was larger as the preoperative spherical refractive error increased and
did not depend on the preoperative internal aberrations. The
correlation coefficient of post-LASIK internal spherical aberration to
pre-LASIK spherical refractive error is 0.73 (P =
0.0024) and of the induced internal spherical aberration (before minus
after surgery) to pre-LASIK spherical refractive error is 0.74
(P = 0.0016). LASIK surgery is not likely to induce
changes in the crystalline lens; the changes therefore seem to occur in
the posterior corneal surface. The effect is only present for spherical
aberration, but not for other terms.
This finding is consistent with recent reports using scanning slit corneal topography. They show posterior corneal surface changes of curvature after PRK for myopia48 and LASIK,49 50 which produce a forward shift of the posterior corneal surface. This suggests that after LASIK and PRK the thinner, ablated cornea may bulge forward slightly, steepening the posterior corneal curvature. This effect has been thought to account for the regression toward myopia that is sometimes found after treatment, particularly in the patients with highest preoperative myopia.48 We used a simple corneal model with aspherical surfaces and found that the observed mean changes of internal spherical aberrations are consistent with the changes in power and asphericity of the posterior corneal surface that have been reported recently. Seitz et al.51 found that the posterior central corneal power changed significantly from -6.28 to -6.39 D after LASIK, and the asphericity power changed from 0.98 to 1.14, in a group of eyes with preoperative spherical refractive error similar to those in our study (range: -1.00 to -15.50, mean, -5.07 ± 2.81 D). For these data, we found that the induced spherical aberration of the posterior corneal surface is -0.103 µmvery similar to the change in internal spherical aberration that we measured experimentally (-0.110 µm, on average).
In summary, using a combination of aberrometry and anterior corneal topography, we showed that this change in the posterior corneal shape also produced a decrease of spherical aberration in comparison with that predicted from anterior corneal aberrations alone. Our results confirm that this biomechanical corneal response is correlated with the amount of preoperative myopia (or, equivalently, with the depth of corneal ablation). From previous studies,49 it is likely that it also depends on the preoperative corneal thickness and intraocular pressure.
Implications
Our results have important implications for the evaluation
outcomes in standard LASIK surgery for myopia, as well as for the
design of wavefront-guided ablation procedures (designed to individual
canceling preoperative aberrations). First, the results show that the
combination of corneal and total aberrations is necessary to understand
individual surgical outcomes and their impact on visual performance. In
general, both corneal and total aberrations increased with surgery, but
the particular increment depended on the individual subject. This is
particularly critical in any aberration-free procedure, which cannot
rely on the mean population response, but must be adapted to the
individual patient. Second, total wavefront aberration measurements
complement corneal topography information to gain insight into the
biomechanical corneal response. Although the ablation is applied on the
anterior corneal surface, our analysis revealed changes in the shape of
the posterior corneal surface, assessed by the modification of its
spherical aberration.
| Acknowledgements |
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| Footnotes |
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Submitted for publication May 23, 2001; revised July 13, 2001; accepted August 2, 2001.
Commercial relationships policy: N.
The publication costs of this article were defrayed in part by page
charge payment. This article must therefore be marked
"advertisement" in accordance with 18 U.S.C.
1734
solely to indicate this fact.
Corresponding author: Susana Marcos, Instituto de Optica, CSIC, Serrano 121, Madrid 28006, Spain. susana{at}io.cfmac.csic.es
| References |
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