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The Effect of Pupil Position on Element Aberration

      Instead of the stop being located at the surface in question, the stop is displaced by a distance, s, from the surface. The chief ray, passing through the centre of the stop defines the field angle, θ. In addition, the pupil co-ordinates defined at the stop are denoted by rx and ry. However, if the stop were located at the optical surface, then the field angle would be θ′, as opposed to θ. In addition, the pupil co-ordinates would be given by rx and ry. Computing the revised third order aberrations proceeds upon the following lines. All the previous analysis, e.g. as per Eqs. (4.31a)(4.31d), has enabled us to express all aberrations as an OPD in terms of θ′, rx, and ry. It is clear that to calculate the aberrations for the new stop locations, one must do so in terms of the new parameters θ, rx, and ry. This is done by effecting a simple linear transformation between the two sets of parameters. Referring to Figure 4.15, it is easy to see:

      (4.40a)equation

Geometrical illustration of the impact of stop movement.

      (4.40c)equation

      (4.41)equation

      In this case, r0 refers to the pupil radius at the stop and r0′ to the effective pupil radius at the surface in question. As a consequence, we can re-cast all three equations in a more convenient form.

      The angle, θ0 is representative of the maximum system field angle and helps to define the eccentricity parameter and the Lagrange invariant. We already know the OPD when cast in terms of rx, ry, and θ, as this is as per the analysis for the case where the stop is at the optic itself. That is to say, the expression for the OPD is as given in Eqs. and these aberrations defined in terms of KSA, KCO, KAS, KFC, and KDI. Therefore, the total OPD attributable to the five Gauss-Seidel aberrations is given by:

      (4.44b)equation