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

✍ Scribed by Paolo Walter Cattaneo


Book ID
103857920
Publisher
Elsevier Science
Year
2009
Tongue
English
Weight
736 KB
Volume
608
Category
Article
ISSN
0168-9002

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✦ Synopsis


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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