Cosmic ray measurements with Pamela experiment (Articolo in rivista)

Type
Label
  • Cosmic ray measurements with Pamela experiment (Articolo in rivista) (literal)
Anno
  • 2009-01-01T00:00:00+01:00 (literal)
Alternative label
  • A.M. Galper, O. Adriani, P. Picozza, G. Castellini, et al. (2009)
    Cosmic ray measurements with Pamela experiment
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • A.M. Galper, O. Adriani, P. Picozza, G. Castellini, et al. (literal)
Pagina inizio
  • 293 (literal)
Pagina fine
  • 299 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 190 (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1. Univ Florence, Dept Phys, I-50019 Florence, Italy 2. INFN, Sez Firenze, I-50019 Florence, Italy 3. Univ Naples Federico 2, Dept Phys, I-80126 Naples, Italy 4. INFN, Sez Napoli, I-80126 Naples, Italy 5. PN Lebedev Phys Inst, RU-119991 Moscow, Russia 6. Univ Bari, Dept Phys, I-70126 Bari, Italy 7. INFN, Sez Bari, I-70126 Bari, Italy 8. INFN, Sez Trieste, I-34149 Trieste, Italy 9. AF Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia 10. INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy 11. Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy 12. Moscow Engn & Phys Inst, RU-11540 Moscow, Russia 13. AlbaNova Univ Ctr, Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden 14. KTH, Dept Phys, SE-10691 Stockholm, Sweden 15. IFAC, I-50019 Florence, Italy 16. Univ Trieste, Dept Phys, I-34147 Trieste, Italy 17. Univ Siegen, Dept Phys, D-57068 Siegen, Germany 18. Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy (literal)
Titolo
  • Cosmic ray measurements with Pamela experiment (literal)
Abstract
  • PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature hi a wide energy range (protons: 80 MeV-700 GeV, electrons 50 MeV-400 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, 15(th) 2006 in a 350 X 600 km orbit with an inclination of 70 degrees. In this work we describe the scientific objectives awl the performance of PAMELA in its first two years of operation. Data oil protons of trapped, secondary and galactic nature - as well as measurements of the December 13(th) 2006 Solar Particle Event - are also provided. (literal)
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