Speaker
Description
The Pierre Auger Observatory is the world's largest detector for the detection of ultra high energy cosmic rays. It is designed as a hybrid detector with a Surface Detector (SD) and a Fluorescence Detector (FD) as its baseline components. The SD consists of 1600 stations, which cover an area of 3000 km
The data read-out of AERA is triggered externally in particular by the SD. This results in many triggers for event that are not relevant for AERA as they are too far away. In addition, not all events of interest yield a trigger. To improve the external trigger, a new reconstruction method for determining the direction of an air shower on trigger level is presented. Based on this method different trigger-conditions are defined and tested. This results in a substantial improvement compared to the current AERA trigger.
Category | Particle / Astroparticle / Cosmology (Experiment) |
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