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Konferenzbeitrag

Simulations of detector arrays and the impact of atmospheric parameters

MPG-Autoren
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Bernloehr,  K.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Volltexte (frei zugänglich)

1402.5081v1
(Preprint), 296KB

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Zitation

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.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0024-E4B1-0
Zusammenfassung
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.