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astro-ph2003
Conceptual Design of a Cosmic Ray Detector Operating Between 10^17 and 10^19 eV for the Study of the Galactic Center
Todd Adams, Eugene C. Loh, Segev BenZvi +1
For our understanding of the origin of ultra high energy cosmic rays, the energy region between 10^17 and 10^19 eV is of crucial importance. Previous experiments have found indirec…
astro-ph1997
CASA-BLANCA: A Large Non-imaging Cherenkov Detector at CASA-MIA
M. Cassidy, L. F. Fortson, J. W. Fowler +5
The lateral distribution of Cherenkov light at ground level records important information on the development of the cosmic ray air shower which produces it. We have constructed an…