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Atmospheric Monitoring for the Pierre Auger Fluorescence Detector
- Source :
- 28th International Cosmic Ray Conference, International Cosmic Ray Conference 28 ICRC 2003, International Cosmic Ray Conference 28 ICRC 2003, Jul 2003, Tsukuba, Japan. pp.465-468, HAL
- Publication Year :
- 2003
- Publisher :
- HAL CCSD, 2003.
-
Abstract
- Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The Auger program for atmospheric monitoring, designed to measure these corrections and to minimize these uncertainties, is summarized in this paper.<br />Four (4) pages, and three (3) EPS figures. Proceedings of the 28th International Cosmic Ray Conference, Universal Academy Press, Inc. Tokyo, Japan, HE (2003) 465-468
- Subjects :
- [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Astrophysics (astro-ph)
FOS: Physical sciences
Astrophysics
Physics::Atmospheric and Oceanic Physics
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- 28th International Cosmic Ray Conference, International Cosmic Ray Conference 28 ICRC 2003, International Cosmic Ray Conference 28 ICRC 2003, Jul 2003, Tsukuba, Japan. pp.465-468, HAL
- Accession number :
- edsair.doi.dedup.....654905306ef5e6d76dc523a19a8dd074