Slide 1 1 UNIVERSITA’ DEL SALENTO Facoltà di Scienze MM.FF.NN TIME MEASUREMENTS WITH THE ARGO-YBJ DETECTOR Dott.ssa Anna Karen Calabrese Melcarne Dottorato di Ricerca…

EUSO The Extreme Universe Space Observatory Marco Pallavicini INFN Genova, Italy Talk Overview Scientific case and Science Goals The observational approach The detector on…

Shock acceleration of cosmic rays Tony Bell Imperial College, London Reynolds, 1986 SNR suitable CR source below 1015eV Typical max. radius of rapidly expanding SNR ~ 1017m…

13 December 2011 The Ohio State University * A Comparison of Energy Spectra in Different Parts of the Sky Carl Pfendner, Segev BenZvi, Stefan Westerhoff University of Wisconsin…

Very Large Volume Neutrino Telescope Workshop Athens 13 â 15 October 2009 Recent Results on Ultra High Energy Cosmic Rays Alan Watson University of Leeds [email protected]…

Gamma Ray Bursts, Supernovae, and the Origin of Cosmic Rays Charles Dermer (Naval Research Laboratory) Erice June, 2002 James Chiang (NASA/GSFC and UMBC) Markus Böttcher…

Neutrino Astronomy at the South Pole David Boersma UW Madison Lake Louise Winter Institute Chicago, 23 February 2006 David Boersma @ Lake Louise Winter Institute 2006 IceCube…

Measurements of Ultra High Energy Cosmic Rays with the Pierre Auger Observatory Lino Miramonti - Kathmandu 14-18 October 2013 1 INTERNATIONAL CONFERENCE ON "Black holes,…

Challenges in Revealing Dark Matter from the High Energy Gamma-Ray Background (Continuum) Ranga-Ram Chary Spitzer Science Center, Caltech [email protected] The Different…

The Highest Energy Paticles from the Sky Angela V. Olinto The University of Chicago Anisotropies at the Highest Energies 6/23/10 1 CMB vs UHECR Anisotropies UHECRS are Charged,…