Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment (Articolo in rivista)

Type
Label
  • Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment (Articolo in rivista) (literal)
Anno
  • 2013-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.3103/S1062873813110221 (literal)
Alternative label
  • Mikhailov V.V.; Adriani O.; Bazilevskaya G.A.; Barbarino G.C.; Belotti R.; Bogomolov E.A.; Boezio M.; Bonvicini V.; Bongi M.; Bonechi L.; Bottai S.; Bruno A.; Vacchi A.; Vannuccini E.; Vasilyev G.I.; Voronov S.A.; Wu J.; Galper A.M.; Grishantseva L.A.; De Santis C.; De Simone N.; Jerse G.; Di Felice V.; Zampa G.; Zampa N.; Zverev V.G.; Casolino M.; Campana D.; Carlson P.; Carbone R.; Karelin A.V.; Castellini G.; Cafagna F.; Kvashnin A.N.; Koldashov S.V.; Koldobskiy S.A.; Consiglio L.; Krutkov S.Y.; Leonov A.A.; Malakhov V.V.; Mayorov A.G.; Malvezzi V.; Marcelli L.; Menn W.; Mocchiutti E.; Monaco A.; Mori N.; Osteria G.; Palma F.; Papini P.; De Pascale M.P.; Pizzolotto C.; Picozza P.; Pearce M.; Rossetto L.; Ricci M.; Ricciarini S.; Sarkar R.; Simon M.; Sparvoli R.; Spillantini P.; Stozhkov Y.I.; Yurkin Y.T. (2013)
    Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment
    in Bulletin of the Russian Academy of Sciences. Physics
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Mikhailov V.V.; Adriani O.; Bazilevskaya G.A.; Barbarino G.C.; Belotti R.; Bogomolov E.A.; Boezio M.; Bonvicini V.; Bongi M.; Bonechi L.; Bottai S.; Bruno A.; Vacchi A.; Vannuccini E.; Vasilyev G.I.; Voronov S.A.; Wu J.; Galper A.M.; Grishantseva L.A.; De Santis C.; De Simone N.; Jerse G.; Di Felice V.; Zampa G.; Zampa N.; Zverev V.G.; Casolino M.; Campana D.; Carlson P.; Carbone R.; Karelin A.V.; Castellini G.; Cafagna F.; Kvashnin A.N.; Koldashov S.V.; Koldobskiy S.A.; Consiglio L.; Krutkov S.Y.; Leonov A.A.; Malakhov V.V.; Mayorov A.G.; Malvezzi V.; Marcelli L.; Menn W.; Mocchiutti E.; Monaco A.; Mori N.; Osteria G.; Palma F.; Papini P.; De Pascale M.P.; Pizzolotto C.; Picozza P.; Pearce M.; Rossetto L.; Ricci M.; Ricciarini S.; Sarkar R.; Simon M.; Sparvoli R.; Spillantini P.; Stozhkov Y.I.; Yurkin Y.T. (literal)
Pagina inizio
  • 1309 (literal)
Pagina fine
  • 1311 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://www.scopus.com/inward/record.url?eid=2-s2.0-84891090939&partnerID=q2rCbXpz (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 77 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo
  • 11 (literal)
Note
  • Scopu (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • INFN Florence and Department of Physics, University of Florence, Florence, 50019, Italy; Lebedev Physics Institute, Russian Academy of Sciences, Moscow, 119991, Russian Federation; INFN Naples and Department of Physics, University of Naples, Naples, 80126, Italy; INFN Bari and Department of Physics, University of Bari, Bari, 70126, Italy; National Nuclear Research University (MEPhI), Moscow, 115409, Russian Federation; Ioffe Physicotechnical Institute, Russian Academy of Sciences, St.-Petersburg, 194021, Russian Federation; INFN Trieste and Department of Physics, University of Trieste, Trieste, 34147, Italy; INFN Rome and Department of Physics, Tor Vergata University of Rome, Rome, 00133, Italy; Department of Physics, Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, Stockholm, 10691, Sweden; Nello Carrara Institute of Applied Physics, Sesto Fiorentino, Florence 50019, Italy; Department of Physics, University of Siegen, Siegen, 57068, Germany; INFN, Frascati National Laboratories, Frascati, 00044, Italy (literal)
Titolo
  • Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment (literal)
Abstract
  • The PAMELA experiment is being conducted aboard the Russian satellite Resurs-DK 1, which was launched into a near-Earth circumpolar orbit on June 15, 2006. The instrument, which includes a magnetic spectrometer and an electromagnetic calorimeter (16X 0), allows us to measure the fluxes of cosmic-ray electrons and positrons over a wide range of energies from ~100 MeV to hundreds of GeV. This work presents the measurement data collected from July 2006 through January 2010 on the spectra of primary cosmic-ray electrons and positrons. At low energies, this spectrum is in good agreement with a diffusion model that includes reacceleration and damping. At high energies, the measured spectrum is harder than the one predicted. © 2013 Allerton Press, Inc. (literal)
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