'Surface detector' presentation slideshows

Cosmic ray anisotropy from Pierre Auger Observatory

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Cosmic ray anisotropy from Pierre Auger Observatory

520 views • 51 slides

Recent results from Pierre Auger Observatory

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Ultrahigh Energy Cosmic Rays at the Pierre Auger Observatory

Ultrahigh Energy Cosmic Rays at the Pierre Auger Observatory. Carl Pfendner December 4, 2008. Knee. Why Study UHECRs?. after Gaisser. Measured spectrum extends to E > 10 20 eV - the highest particle energies observed in the Universe. Cosmic ray energy spectrum is nonthermal:

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Fermilab Program Advisory Committee

371 views • 25 slides

Recent results from the Pierre Auger Observatory

Recent results from the Pierre Auger Observatory. Pham Ngoc Diep for the Pierre Auger Observatory. Vinh 10/2011. x = 2.7. x = 3.0. x = 2.7. Cosmic rays. charged particles, extremely high energies ~10 20 eV=16 Joules! power law spectrum ~ E -2.7 Galactic: DSA in young SNR shells

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Status of the Pierre Auger Observatory

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Future Plans at the Pierre Auger Observatory

Future Plans at the Pierre Auger Observatory. Lawrence Wiencke Colorado School of Mines IS@AO, Apr. 18 2011, Cambridge. Logarithmic Scale. Linear Scale. Linsleys. x10 5 Linsleys. TA. Wiencke. Southern site: Argentina. Argentina Australia Brasil Bolivia* Czech Rep.

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A possible origin of ultra-high energy cosmic rays: collisions of two galaxies

41 views • 2 slides

A possible origin of ultra-high energy cosmic rays: collisions of two galaxies

131 views • 2 slides