Optical analysis of spherical mirrors of telescopes: the lens-less Schmidt case

Details Optical analysis of spherical mirrors of telescopes: the lens-less Schmidt case Optical analysis of spherical mirrors of telescopes: the lens-less Schmidt case

2009-08-25

arxiv.org/abs/0908.3646v1

Nuclear Instruments and Methods in Physics Research A, 608/3 (2009) 394-389

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

20 pages, 6 figures, accepted by Nuclear Instruments and Methods in Physics Research

Scientific paper

10.1016/j.nima.2009.07.032

The light distribution on the focal surface of spheric mirrors designed for
telescopes in the lens-less Schmidt configuration is calculated analytically
using geometrical optics. This analysis was motivated by considerations of the
design the design of the AUGER fluorescence detector. Its geometrical
parameters are used in the examples.

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