When this research was performed the author was with the Division of Materials Science and Technology, Commonwealth Scientific and Industrial Research Organisation, Normanby Road, Clayton, Victoria 3168, Australia. He is now with Prime Optics, 17 Crescent Road, Eumundi, Queensland 4562, Australia.
A wide-field (2°) prime focus corrector has been designed and built for the Anglo-Australian Telescope. The corrector incorporates an atmospheric dispersion compensator for the spectral range 365–1014 nm. A four-element lens system is the basis of the corrector, and it provides a satisfactory state of correction over a full field of 2°. The design of the lens system is described. The choice of layout is related directly to the intrinsic properties of each component.
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A negative radius implies a surface concave to the incident light; a positive radius implies a surface convex to the incident light.
This is the vertex radius of curvature of the hyperboloidal primary mirror, which has a conic constant of −1.1717.
The surfaces of the ADC (surfaces 2, 3, 6, and 7) are configured for a zenith angle of 60° and have their plane of symmetry parallel to the zenith meridian. For a zenith angle of 0°, the signs of the tilts of surfaces 6 and 7 change and the plane of symmetry becomes perpendicular to the zenith meridian.
The optical cement between the elements of the two doublets is assumed to have a constant refractive index of 1.539. Chromatic effects from the thin cement layers will be relatively negligible.
A negative radius implies a surface concave to the incident light; a positive radius implies a surface convex to the incident light.
This is the vertex radius of curvature of the hyperboloidal primary mirror, which has a conic constant of −1.1717.
The surfaces of the ADC (surfaces 2, 3, 6, and 7) are configured for a zenith angle of 60° and have their plane of symmetry parallel to the zenith meridian. For a zenith angle of 0°, the signs of the tilts of surfaces 6 and 7 change and the plane of symmetry becomes perpendicular to the zenith meridian.
The optical cement between the elements of the two doublets is assumed to have a constant refractive index of 1.539. Chromatic effects from the thin cement layers will be relatively negligible.