The High Resolution Fly's Eye - Status and Preliminary Results on Cosmic Ray Composition Above 1018 eV

Details The High Resolution Fly's Eye - Status and Preliminary Results on Cosmic Ray Composition Above 1018 eV The High Resolution Fly's Eye - Status and Preliminary Results on Cosmic Ray Composition Above 1018 eV

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4858..103s&link_type=abstract

Particle Astrophysics Instrumentation. Edited by Peter W. Gorham. Proceedings of the SPIE, Volume 4858, pp. 103-114 (2003).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We describe the current status of the High Resolution Fly's Eye detector. Event reconstruction and associated systematics for stereo reconstruction are discussed and recent preliminary results on the study of the composition of ultra-high energy cosmic rays by the Xmax method are presented. These results indicate that the composition of cosmic rays becomes predominantly light near 1019 eV and beyond.

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