Speaker
Mr
Philipp Julian Rauscher
(Institute for Nuclear Physics Karlsruhe Institute of Technology)
Description
The Pierre Auger Observatory in Argentina aims to survey properties of cosmic rays. The signal of the surface detector array is used to determine the energy of a cosmic ray. It is described by an NKG-type lateral distribution function. A global fit of the parameters on all data of the SD-array shall improve our empirical parameters.
Primary authors
Mr
Philipp Julian Rauscher
(Institute for Nuclear Physics Karlsruhe Institute of Technology)
Dr
Darko Veberiċ
(Institute for Nuclear Physics Karlsruhe Institute of Technology)
Dr
Markus Roth
(Institute for Nuclear Physics Karlsruhe Institute of Technology)
