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EnglishPAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons: 80 MeV–1200 GeV, electrons 50 MeV–600 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV–190 GeV), positrons (50 MeV–270 GeV) and search for antinuclei (with a precision of the order of 10−8). The experiment, housed on board the Russian Resurs-DK1 satellite, was launched on June, 15th 2006 in a 350 × 600 km orbit with an inclination of 70°. In this work we report on the recent results on proton and helium of galactic origin, their solar modulation and the helium isotopic component.
| Titolo: | PAMELA recent results on galactic proton and helium | |
| Autori: | ||
| Data di pubblicazione: | 2011 | |
| Abstract: | PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons: 80 MeV–1200 GeV, electrons 50 MeV–600 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV–190 GeV), positrons (50 MeV–270 GeV) and search for antinuclei (with a precision of the order of 10−8). The experiment, housed on board the Russian Resurs-DK1 satellite, was launched on June, 15th 2006 in a 350 × 600 km orbit with an inclination of 70°. In this work we report on the recent results on proton and helium of galactic origin, their solar modulation and the helium isotopic component. | |
| Handle: | http://hdl.handle.net/11368/2719389 | |
| Appare nelle tipologie: | 4.1 Contributo in Atti Convegno (Proceeding) |
