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  Simulations of detector arrays and the impact of atmospheric parameters

Bernloehr, K. (2014). Simulations of detector arrays and the impact of atmospheric parameters. In Proceedings of the Atmospheric Monitoring for High-Energy Astroparticle Detectors (AtmoHEAD) Conference. Retrieved from http://arxiv.org/abs/1403.4816.

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1402.5081v1 (Preprint), 296KB
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1402.5081v1
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Bernloehr, K.1, Author           
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1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              

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Free keywords: Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,High Energy Physics - Experiment, hep-ex, Physics, Atmospheric and Oceanic Physics, physics.ao-ph
 MPINP: CTA - Abteilung Hofmann
 Abstract: In Monte-Carlo simulations of gamma-ray or cosmic-ray detector arrays on the ground (here mainly arrays of imaging atmospheric Cherenkov telescopes), the atmosphere enters in several ways: in the development of the particle showers, in the emission of light by shower particles, and in the propagation of Cherenkov light (or fluorescence light or of particles) down to ground level. Relevant parameters and their typical impact on energy scale and so on are discussed here.

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 Dates: 2014
 Publication Status: Published online
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 Rev. Type: -
 Identifiers: arXiv: 1403.4816
URI: http://arxiv.org/abs/1403.4816
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Title: Atmospheric Monitoring for High-Energy Astroparticle Detectors (AtmoHEAD) Conference
Place of Event: Saclay, France
Start-/End Date: 2013-07-10 - 2013-07-12

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Title: Proceedings of the Atmospheric Monitoring for High-Energy Astroparticle Detectors (AtmoHEAD) Conference
Source Genre: Proceedings
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Pages: - Volume / Issue: - Sequence Number: 1402.5081 Start / End Page: - Identifier: -