How to Measure Aberrations

Optical designers use different methods to measure optical performance. This mostly consists of measuring optical aberrations. If you are unfamiliar with optical aberrations, please visit our aberrations page. Measuring ray aberrations are one way to evaluate optical system performance and it is fairly intuitive, so let’s start with that.

Ray Aberrations

There are a few common ways that optical designers quantify aberrations. One way is to measure the distance on the image plane that a real ray differs from the ideal image point. This distance is called the “transverse ray aberration” (TRA) as seen in Figure 2.1.

Another way to quantify the aberration is the longitudinal distance (distance along the optical axis) from the ideal image plane to the intersection of the marginal ray with the optical axis. This distance is called the “longitudinal ray aberration” (LRA).

Figure 2.1 Spherical Aberration and Longitudinal Ray Aberrations

Figure 2.1 Transverse and Longitudinal Ray Aberrations

These methods of aberration measurement can be plotted to help with aberration analysis. The transverse ray aberration is generally plotted against normalized pupil coordinates, as shown in Figure 2.2. When this is the case the plot is called a “Ray Fan”. In the ray fan below it can be seen how the points on the fan correspond to the normalized pupil coordinates and the real ray locations on the image plane (a-e) in Figure 2.1.

The longitudinal ray aberration is generally plotted on the x-axis and the normalized pupil coordinate is plotted on the y-axis as seen in Figure 2.3. As with the Ray Fan plot, it can easily be seen how this plot is generated by considering points c, f and g on Figure 1.

In both of these cases, a perfect lens with absolutely zero aberration would result in all of the rays landing on the same point on the image plane. This would result in a straight horizontal line collinear with the x-axis in the ray fan plot and a straight vertical line located at the “0” position in the longitudinal ray aberration plot.

Figure 2: Ray Fan

Figure 2.2: Ray Fan

Another method of plotting is called the Spot Diagram. This plot represents rays from a point source that fill the entrance pupil in all directions and land on the image plane after going through the system. A perfect lens would produce just one point in the spot diagram since all the rays would be imaged to the same location.

Figure 3: Longitudinal Ray Aberration Plot

Figure 2.3: Longitudinal Ray Aberration Plot

Figure 2.4 represents a spot diagram. It can be seen how this diagram is generated by considering the ray locations on the image plane (a-e) in Figure 1. If these ray locations are rotated about the optical axis, the image would result in a center spot with concentric rings surrounding it, which is just what we have in Figure 2.4.

Figure 4: Spot Diagram

Figure 2.4: Spot Diagram

Figure 2.5 represents spot diagrams for different image plane locations and is called a “Through Focus Spot Diagram”. Considering the location of the paraxial image plane in Figure 2.1, it can be seen that the spot generated at this image location will not have the optimal spot size. If the image plane were to be moved closer to the lens to the smallest spot size (represented as the center plot in Figure 2.5) the least amount of aberration will be present.

Figure 5: Through Focus Spot Diagram

Figure 2.5: Through Focus Spot Diagram

Wavefront Aberrations (Coming Soon)