Graciela B. Gelmini
Published 2009-03-26Version 1
I review here some of the physics we are learning and expect to learn in the near future through the observation of cosmic rays. The study of cosmic rays involves a combination of data from accelerators, ground arrays, atmospheric fluorescence detectors and balloon and satellite experiments. I will discuss the data of the Pierre Auger Observatory, PAMELA, ATIC and FST among other experiments.
Comments: 18 pages, 18 figures (iopams.sty, jpconf11.clo and jpconf.cls required to tex). Plenary talk at "Discrete `08", December 11-16 2008, Valencia, Spain
Journal: J.Phys.Conf.Ser.171:012012,2009
The Fortuitous Latitude of the Pierre Auger Observatory and Telescope Array for Reconstructing the Quadrupole Moment
Investigation of Hadronic Interactions at Ultra-High Energies with the Pierre Auger Observatory
$X_{max}^μ$ vs. $N^μ$ from Extensive Air Showers as estimator for the mass of primary UHECR's. Application for the Pierre Auger Observatory
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