The files containing information about corneal elevation were downloaded on removable media and used for the following analysis. The calculation of wavefront aberrations was performed by expanding the anterior corneal height data into the set of orthogonal Zernike polynomials.
8 9 10 The first six Zernike polynomials (
Z 0 0,
Z 1 −1,
Z 1 1,
Z 2 −2,
Z 2 0,
Z 2 2) represent fundamental corneal shapes, such as its base curvature, astigmatism, and any planar tilt. These polynomials were subtracted from the original height data to form a residual height map, and Zernike coefficients 7 through 28 (
Z 3 −3 through
Z 6 6) were computed. Coefficients
Z 3 −3 through
Z 3 3 correspond to coma-like aberrations,
Z 4 −4 through
Z 4 4 correspond to spherical-like aberrations,
Z 5 −5 through
Z 5 5 express the fifth-order Zernike coefficients, and
Z 6 −6 through
Z 6 6 are the sixth-order Zernike coefficients. These Zernike coefficients were used to calculate the global descriptors of monochromatic corneal aberrations, which are represented by the terms
S 3,
S 4,
S 5, and
S 6. Because spherical and coma aberrations refer to symmetrical systems and the eye is not rotationally symmetrical, the terms spherical-like and coma-like aberrations are used in this article. The
S 3 (third-order component of the wavefront aberration) represents the root mean squared wavefront variance from that of a perfect spherocylinder, due to coma-like aberration. Similarly,
S 4 (fourth-order component of the wavefront aberration) represents the root mean squared wavefront variance from that of a perfect spherocylinder, due to spherical-like aberration. The
S 5 and
S 6 are the fifth- and sixth-order components of the wavefront aberration, respectively. Because the variances of each term are independent, the odd-order aberrations were summed (root mean square of
S 3 and
S 5) to examine the magnitude of coma-like aberrations, and the even-order aberrations were summed (root mean square of
S 4 and
S 6) to evaluate the changes in spherical-like aberrations. These calculations were performed for the central circular area of the cornea corresponding to the apparent pupillary diameter of individual eyes, measured as described.