'Cr flux' presentation slideshows

Results from the Pierre Auger Observatory

699 views • 57 slides

Magnetic field and accelerated shock acceleration

Magnetic field and accelerated shock acceleration. Tony Bell Imperial College, London. Lucek & Bell, MNRAS 314, 65 (2000) Bell & Lucek, MNRAS 321, 433 (2001) Bell, MNRAS 353, 550 (2004) Bell, MNRAS 358,181 (2005). SNR suitable CR source below 10 15 eV. x-ray image of SN1006.

502 views • 40 slides

Magnetic field and accelerated shock acceleration

Magnetic field and accelerated shock acceleration. Tony Bell Imperial College, London. Lucek & Bell, MNRAS 314, 65 (2000) Bell & Lucek, MNRAS 321, 433 (2001) Bell, MNRAS 353, 550 (2004) Bell, MNRAS 358,181 (2005). SNR suitable CR source below 10 15 eV. x-ray image of SN1006.

407 views • 40 slides

IceCube non-detection of GRB Neutrinos: Constraints on the fireball properties

Liverpool GRB meeting June 20, 2012. IceCube non-detection of GRB Neutrinos: Constraints on the fireball properties. Xiang-Yu Wang Nanjing University, China Collaborators ? H. N. He, R. Y. Liu, S. Nagataki, K. Murase, Z.G. Dai. High-energy neutrino- a new window. MeV neutrinos: detected

380 views • 29 slides

Gamma-ray emission from molecular clouds: a probe of cosmic ray origin and propagation

Gamma-ray emission from molecular clouds: a probe of cosmic ray origin and propagation. Sabrina Casanova Ruhr Universitaet Bochum & MPIK Heidelberg, Germany. 32nd Int. School of Nucl Physics, Erice Sept 2010. Outline. The Standard Model of Cosmic Rays

574 views • 28 slides

M. Spurio, G. Carminati, A. Margiotta University of Bologna and INFN

MU ons from PA rametric formulas: a fast Ge nerator of atmospheric m for neutrino telescopes ( MUPAGE ). M. Spurio, G. Carminati, A. Margiotta University of Bologna and INFN. VLVnT08 - Toulon 22-24 April 2008. Atmospheric muons in a VLV n T.

424 views • 21 slides

Results from Cosmic-Ray Experiments

Vasiliki Pavlidou Kavli Institute for Cosmological Physics, The University of Chicago. Results from Cosmic-Ray Experiments. Outline. Ultra-high--energy cosmic-rays: issues and detection techniques A hybrid experiment: the Pierre Auger Observatory

327 views • 20 slides

Recurrent Cosmic Ray Variations in 2007-2008

251 views • 18 slides

Can Solar 6 Li Really Be Explained by Galactic Cosmic Rays?

Can Solar 6 Li Really Be Explained by Galactic Cosmic Rays?. Tijana Prodanovi? University of Novi Sad, Serbia Brian D. Fields University of Illinois at Urbana-Champaign. July 5 th , 200 7 30 th ICRC, Merida, Mexico. Outline.

198 views • 8 slides