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Published byElisabeth Server Modified over 9 years ago
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Physics of (and behind) The Roland Maze Project Main goal: UHECR studies (EeV scale) but also (GeV scale): Solar System flares, Furbush decreases, magnetic stroms etc. (TeV scale): GRB (PeV scale): High energy interaction model tests
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Ultra High Energy Cosmic Rays GZK-cutoff
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Ultra High Energy Cosmic Rays GZK-cutoff ?
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Solar System Physics
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Lodz 1 m scyntyllator neutron monitor 2
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CR and weather 11 year cycle
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CR and climate long term variability
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Gamma Ray Bursts
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GRB970417a Milagrito
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GRB970417a
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(2σ limits)
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Distant correlations
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Maze and others
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Roland Maze
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Pierre Auger Observatory
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GZK-cutoff Physics of (and behind) The Roland Maze Project
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