Auger North - Fermilab Center for Particle Astrophysics

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Auger North Objectives! Obtain the greatly expanded data set needed to solve the puzzles of the sources and primary composition.! Extend coverage to the northern sky.!
Larger Aperture for the Auger Observatory! Possibilities! Auger South ! 3000 km 2 at the current site could be expanded to 5000 km 2. ! 20,000 km 2 in a remote area! Auger North! 20,000 + km 2 in SW Colorado ! Full Sky coverage!
Page 1 and 2: The Pierre Auger Observatory Auger
Page 3 and 4: To Discover UHECR Sources ! need:!
Page 5 and 6: Auger South!
Page 7 and 8: Auger South! Observed the GZK featu
Page 9 and 10: Attenuation length! e + e - π Atte
Page 11 and 12: Horizons:! 10 19 eV ~ 1 Gpc! 100 Mp
Page 14 and 15: Recent Auger Spectrum!
Page 18 and 19: Auger VCV correlation! 27 events te
Page 20 and 21: First 27 events!
Page 22 and 23: UHE neutrino limit!
Page 26 and 27: Composition observable: ! shower ma
Page 28 and 29: Puzzling Composition! Unexpected As
Page 30 and 31: Neutrino Fluxes!
Page 32 and 33: Above 60 EeV: ! either Protons or I
Page 34 and 35: If Correlated with sources ! < 10 o
Page 36 and 37: Hadronic Interactions ! Parameters
Page 40 and 41: Auger North - 10 yr Auger South - 1
Page 42 and 43: FD disentangle Composition !
Page 44 and 45: Galactic Plane!
Page 46 and 47: Determine Source Distribution! Type
Page 48 and 49: Lindsleys Exposure Evolution - Line
Page 52 and 53: State of Colorado Auger North: 4000
Page 54 and 55: Features of Auger North Fluorescenc
Page 56 and 57: Communications System Campus Area M
Page 58 and 59: Argentina " "Netherlands! Australia
Page 60 and 61: Estimated Construction Cost! WBS Ac
Page 62 and 63: Funding! Auger South ($54M):! Europ
Page 64 and 65: US Auger Groups! Argonne National L
Page 66 and 67: The Pierre Auger Observatory Auger
Page 68 and 69: Auger North Auger South Auger North

Auger North - Fermilab Center for Particle Astrophysics

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