'5 gv' presentation slideshows

La missione PAMELA: primi risultati scientifici

793 views • 63 slides

Outline of the lecture

Outline of the lecture. Lecture 2: Sources of background and their rejection Efficiencies & Contaminations Absolute fluxes Conclusions. Lecture 2: Sources of background and their rejection. Antiprotons. High-energy antiproton analysis. Antiproton/proton identification :

781 views • 60 slides

Observational data on Primary CR Spectrum

Observational data on Primary CR Spectrum. from here c = 1. CR composition at low energies. Particle abundances in CR (at E > 2.5 GeV/particle, minimum SA) and in Universe.

680 views • 59 slides

Observational data on Primary CR Spectrum

Observational data on Primary CR Spectrum. from here c = 1. CR composition at low energies. Particle abundances in CR (at E > 2.5 GeV/particle, minimum SA) and in Universe.

593 views • 59 slides

Results from the PAMELA space experiment

633 views • 44 slides

High-Energy Ground Level Events Measured with Neutron Monitors and the Milagro Instrument

High-Energy Ground Level Events Measured with Neutron Monitors and the Milagro Instrument. James M. Ryan University of New Hampshire and the Milagro Collaboration. The Network. Northeast US Mount Washington IGY; P c = 1.68 GV; 2028 m Durham NM64; P c = 1.88 GV; sea level

144 views • 14 slides