Towards the identification of the primary particle nature by the radiodetection method with the CODALEMA experiment
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Web: Contact: [email protected] HAWC is a collaborative effort between institutions in the United States of America.
Proposal Submitted to NSF/DoE HEP Given the large increase in sensitivity for a moderate cost, we have decided to propose to build HAWC. A proposal was.
TeV Observations Of Diffuse Emission Probing Galactic Gamma-Ray Sources Brenda Dingus Los Alamos National Lab Milagro: A Diffuse TeV Observatory TeV Gamma-Ray.
The First Flight of EUSO Balloon a prototype of JEM-EUSO Jim Adams a, Evgeny Kuznetsov a, Matthew Rodencal a, Jurgen Sawatzki a, Mark Christl b, Lawrence.
Ultra High Energy Cosmic Rays Glennys R. Farrar Center for Cosmology and Particle Physics, Department of Physics, New York University.
Cosmic Rays Liz Puchnarewicz Mullard Space Science Laboratory University College London .
HIGH-SPEED HARDWARE RANDOM NUMBER GENERATOR Using Geiger mode photo detector Presented by: Dr. Dmitriy Beznosko, Physics Dept., SST, NU 1.
Size and Energy Spectra of incident cosmic radiation obtained by the MAKET - ANI surface array on mountain Aragats. (Final results from MAKET-ANI detector)
The First Flight of EUSO Balloon a prototype of JEM-EUSO
