physics of (and behind) the roland maze project
DESCRIPTION
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. Ultra High Energy Cosmic Rays. GZK-cutoff. - PowerPoint PPT PresentationTRANSCRIPT
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
Ultra High Energy Cosmic Rays
GZK-cutoff
Ultra High Energy Cosmic Rays
GZK-cutoff
?
Solar System Physics
Solar System Physics
Lodz 1 m scyntyllator
neutron monitor
2
CR and weather
11 year cycle
CR and climate
long term variability
Gamma Ray Bursts
GRB970417a
Milagrito
GRB970417a
GRB970417a
(2σ limits)
Distant correlations
Maze and others
Roland Maze
Pierre Auger Observatory
GZK-cutoff
Physics of (and behind) The Roland Maze Project