1. Transverse tangential coma (TTC), described for marginal, meridional rays and paraboloid mirrors by TTC y =− 3 2 κθ2, (8.17) is a blurring aberration, as is spherical aberration, because the dependence upon y brings rays incident at =
Any paraboloid (elliptic or hyperbolic) is a translation surface, as it can be generated by a moving parabola directed by a second parabola. Properties and applications. Elliptic paraboloid. Polygon mesh of a circular paraboloid. Circular paraboloid. In a suitable Cartesian coordinate system, an elliptic paraboloid has the equation.
The surface of revolution obtained from an ellipse is called an ellipsoid, and that obtained from a parabola is called a paraboloid. A hyperbola gives rise to different surfaces of revolution, depending on whether it is revolved about the conjugate axis (which passes between the two branches of the hyperbola) or the transverse axis (which ...
how to trace their standard forms. We shall trace an elliptic paraboloid hc I(. .iilcl leave the tracing of a hyperbolic paraboloid as an exercise for you. So, let us consider (S), the standard equation of an elliptic paraboloid. We can observe some geometrical properties, similar to the properties you have seen in Unit 8
Transverse ray aberration (TRA) expansions are expressed as functions of entrance aperture coordinates (h, β) shown in Figure 2. The expansions presented here are based on the format introduced by Cox16. The derivation is simple but rather lengthy. In the derivation an off-axis ray making an angle δ is mathematically traced from the primary
2023年9月1日 · We define the transverse spherical aberration (TSA), as the intersection of a ray from height r on the mirror with the paraxial focal plane, as shown in Fig. 4.2. It is conventional to define the longitudinal spherical aberration (LSA), as the distance from the paraxial focal plane to the point where a ray from height r crosses the z-axis.
Transverse ray aberration expansions are derived for a paraboloid–hyperboloid telescope. The expansions are valid for glancing incidence Wolter type II and normal incidence Cassegrain telescopes. The analysis gives all third-order aberration terms except distortion and four fifth-order aberration terms as a function of the system parameters ...
The elliptical paraboloid described by equation 4.1.6 is easy to visualize. Slightly less easy (but by no means unreasonably difficult) to visualize is a hyperbolic paraboloid ,