Slide 1 (2) Profile of the Non-Thermal Filaments of SNRs =>High Energy Particle Acceleration =>High Energy Particle Acceleration In all the SNRs & GC Non Thermal…

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…

Radio and X-Ray Properties of Magellanic Cloud Supernova Remnants John R. Dickel Univ. of Illinois with: D. Milne. R. Williams, V. McIntyre, J. Lazendic, Y.-H. Chu, R. Gruendl,…

Origin of high-energy cosmic rays Vladimir Ptuskin IZMIRAN knee Galactic extragalactic GZK cutoff JXE3 Ncr ~ 10-10 cm-3 - total number density in the Galaxy wcr ~ 1.5 eV/cm3…

Magnetic field and accelerated shock acceleration Tony Bell Imperial College, London Lucek & Bell, MNRAS 314, 65 (2000) Bell & Lucek, MNRAS 321, 433 (2001) Bell,…

Origin of high-energy cosmic rays Vladimir Ptuskin IZMIRAN knee Galactic extragalactic GZK cutoff JXE3 Ncr ~ 10-10 cm-3 - total number density in the Galaxy wcr ~ 1.5 eV/cm3…

Radio and X-Ray Properties of Magellanic Cloud Supernova Remnants John R. Dickel Univ. of Illinois with: D. Milne. R. Williams, V. McIntyre, J. Lazendic, Y.-H. Chu, R. Gruendl,…