Login

4th Workshop on Air Shower Detection at High Altitude

31 January 2013 to 1 February 2013
Napoli
Europe/Rome timezone
Important news: please have a look at the Accommodation Info page

Support

Session

GZK and below

31 Jan 2013, 16:20
Aula Magna Partenope (Napoli)

Aula Magna Partenope

Napoli

Centro Congressi Partenope Via Partenope 36, Napoli

Presentation materials

There are no materials yet.

  1. 11. The Pierre Auger Observatory and its performance
    Dr Corinne Berat (Laboratoire de Physique Subatomique et de Cosmologie (LPSC))
    31/01/2013, 16:20
    Ultra High Energy Cosmic Rays (UHECR) represent the most energetic elementary particles available to scientists. They have macroscopic energies, exceeding 1 EeV, but their flux is very weak, one particle per century per square kilometre for the highest energies. Understanding their nature and origin is the objective of the Pierre Auger Observatory, which is located in the province of Mendoza...
    Go to contribution page
  2. 10. Recent results from the Pierre Auger Observatory
    Lorenzo Perrone (LE)
    31/01/2013, 16:50
  3. 14. Telescope Array
    Douglas Bergman
    31/01/2013, 17:20
  4. 33. Radioactive UHECR decaying in the sky painting TEV anisotropies
    Prof. Daniele Fargion (ROMA1)
    31/01/2013, 17:50
Building timetable...