Optical analysis of spherical mirrors of telescopes: The lens-less Schmidt case
作者: Paolo Walter Cattaneo
作者单位: 1INFN Pavia, Via Bassi 6, 27100 Pavia, Italy
刊名: Nuclear Inst. and Methods in Physics Research, A, 2009, Vol.608 (3), pp.384-389
来源数据库: Elsevier Journal
DOI: 10.1016/j.nima.2009.07.032
关键词: Cosmic ray detectorsGeometrical optics
英文摘要: Abstract(#br)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.(#br)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.
全文获取路径: Elsevier  (合作)