Orateur
Dr
Konrad Bernlöhr
(MPIK Heidelberg)
Description
In Monte-Carlo simulations of detector arrays on the ground (here mainly arrays of 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 etc. will be discussed.
Auteur principal
Dr
Konrad Bernlöhr
(MPIK Heidelberg)
