Published May 30, 2001
| Version v1
Journal article
Optical design of the fluorescence detector telescopes
Description
It is reported the optical design of the Auger and Kosmotepetl projects. For the first one it was used a Schmidt camera without corrector plate and for the second one it is proposed to use a Fresnel mirror of low frequency with a stop located at the common curvature center in order to avoid the coma and astigmatism aberrations
Additional details
Identifiers
- DOI
- 10.1063/1.1378624;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 566
- Journal Issue
- 1
- Journal Page Range
- p. 91-98
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- International workshop on observing ultra high energy cosmic rays from space and earth
- Dates
- 9-12 Aug 2000
- Place
- Metepec, Puebla (Mexico)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35052790
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CAMERAS; COSMIC RAY DETECTION; COSMIC RAY SPECTROMETERS; FRESNEL REFLECTORS; MIRRORS; PARTICLE DISCRIMINATION
- Descriptors DEC
- DETECTION; EQUIPMENT; MEASURING INSTRUMENTS; MIRRORS; PARTICLE IDENTIFICATION; RADIATION DETECTION; SOLAR CONCENTRATORS; SOLAR EQUIPMENT; SOLAR REFLECTORS; SPECTROMETERS
Optional Information
- Notes
- (c) 2001 American Institute of Physics.