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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.
Pierre Sokolsky
"The High Resolution Fly's Eye - Status and Preliminary Results on Cosmic Ray Composition Above 1018 eV", Proc. SPIE 4858, Particle Astrophysics Instrumentation, (3 March 2003); https://doi.org/10.1117/12.477965
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Pierre Sokolsky, "The High-Resolution Fly's Eye: status and preliminary results on cosmic ray compositition above 10 (18) eV," Proc. SPIE 4858, Particle Astrophysics Instrumentation, (3 March 2003); https://doi.org/10.1117/12.477965