Feb 13 – 16, 2012
Europe/Zurich timezone

Disentangling the Air Shower Components Using Scintillator and Water Cherenkov Detectors.

Not scheduled
500/1-001 - Main Auditorium (CERN)

500/1-001 - Main Auditorium


CERN, Geneva
Show room on map


Javier G. Gonzalez (KIT)


The current challenge in studying ultra-high energy cosmic rays is inferring the primary mass-composition. In order to get a better handle on mass-composition it is vital that we disentangle the contributions from the different components of the air shower, as this relates to the primary mass as well as possible systematic uncertainties arising from the use of Monte Carlo hadronic interaction generators. We therefore consider a ground array of scintillator and water Cherenkov detectors. The different response characteristics of these two types of detectors to the components of the air shower could provide a way to infer their relative contributions. We use a detailed simulation in order to estimate the impact of parameters, such as scintillator detector size, in the determination of the size of the muon component.

Primary author


Dr Markus Roth (KIT) Dr Ralph Engel (Forschungszentrum Karlsruhe)

Presentation materials

There are no materials yet.