The CONDOR Observatory layout is being optimized
It will consist of an array of detectors that will measure the particles being produced in the interaction of cosmic rays and the upper atmosphere.
When gamma rays hit the upper atmosphere, they produce a "shower" of secondary particles that can be measured at ground level. Below are shown some examples of showers obtained with a simulation program (CORSIKA) for different energies:
50 GeV gamma ray
100 GeV gamma ray
1000 GeV gamma ray
