Atmospheric monitoring and model applications at the Pierre Auger Observatory

B. KEILHAUER; THE PIERRE AUGER COLLABORATION.; S. J. SCIUTTO

Roma

Conferencia; AtmoHEAD 2014 Conference; 2014

The Pierre Auger Observatory detects high-energy cosmic rays with energies above∼1017eV. It is built as a multi-hybrid detector measuring extensive air showers with different techniques. For the reconstruction of extensive air showers, theatmospheric conditions at the site of the Observatory have to be known quite well. This is particularly true for reconstructionsbased on data obtained by the fluorescence technique. For these data, not only the weather conditions near ground are relevant,most important are altitude-dependent atmospheric profiles. The Pierre Auger Observatory has set up a dedicated atmosphericmonitoring programme at the site in the Mendoza province, Argentina. Beyond this, exploratory studies were performed inColorado, USA, for possible installations in the northern hemisphere. In recent years, the atmospheric monitoring programmeat the Pierre Auger Observatory was supplemented by applying data from atmospheric models. Both GDAS and HYSPLIT aredevelopments by the US weather department NOAA and the data are freely available. GDAS is a global model of the atmosphericstate parameters on a 1 degree geographical grid, based on real-time measurements and numeric weather predictions, providing afull altitude-dependent data set every 3 hours. HYSPLIT is a powerful tool to track the movement of air masses at various heights,and with it the aerosols. Combining local measurements of the atmospheric state variables and aerosol scattering with the givenmodel data, advanced studies about atmospheric conditions can be performed and high precision air shower reconstructions areachieved.