Optical analysis of spherical mirrors of telescopes: The lens-less Schmidt case |
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| Authors: | Paolo Walter Cattaneo |
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| Affiliation: | aINFN Pavia, Via Bassi 6, 27100 Pavia, Italy |
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| Abstract: | 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 of the AUGER fluorescence detector [J. Abraham, et al., Nucl. Instr. and Meth. A 533 (2004) 50]. Its geometrical parameters are used in the examples. |
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| Keywords: | Cosmic ray detectors Geometrical optics |
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