Future projects for the highest energy cosmic rays

Details Future projects for the highest energy cosmic rays Future projects for the highest energy cosmic rays

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.620t&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The discovery of the highest energy cosmic rays above 1020eV by Fly's Eye and AGASA experiments gave us a strong motivation to propose next generation detectors. The detection techniques for the highest energy cosmic rays, and the future projects (Auger, TA/snake, OWL/Air Watch) will be reviewed. In order to clarify the source of these energetic cosmic rays, the capabilities of neutrino detection and the primary particle identification become essential. The characteristics of showers induced by neutrinos and gammas are also discussed.

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