Measurement of hydrogen and helium isotopes flux in galactic cosmic rays with the PAMELA experiment (Articolo in rivista)

Type
Label
  • Measurement of hydrogen and helium isotopes flux in galactic cosmic rays with the PAMELA experiment (Articolo in rivista) (literal)
Anno
  • 2014-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1016/j.nima.2013.11.004 (literal)
Alternative label
  • Formato V.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bongi M.; Bonvicini V.; Bottai S.; Bruno A.; Cafagna F.; Campana D.; Carbone R.; Carlson P.; Casolino M.; Castellini G.; De Donato C.; De Pascale M.P.; De Santis C.; De Simone N.; Di Felice V.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobskiy S.; Krutkov Y.; Kvashnin A.N.; Leonov A.; Malakhov V.; Marcelli L.; Martucci M.; Mayorov A.G.; Menn W.; Merge M.; Mikhailov V.V.; Mocchiutti E.; Monaco A.; Mori N.; Munini R.; Osteria G.; Palma F.; Papini P.; Pearce M.; Picozza P.; Pizzolotto C.; Ricci M.; Ricciarini S.B.; Sarkar R.; Simon M.; Scotti V.; Sparvoli R.; Spillantini P.; Stozhkov Y.I.; Vacchi A.; Vannuccini E.; Vasilyev G.; Voronov S.A.; Yurkin Y.T.; Zampa G.; Zampa N.; Zverev V.G. (2014)
    Measurement of hydrogen and helium isotopes flux in galactic cosmic rays with the PAMELA experiment
    in NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Formato V.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bongi M.; Bonvicini V.; Bottai S.; Bruno A.; Cafagna F.; Campana D.; Carbone R.; Carlson P.; Casolino M.; Castellini G.; De Donato C.; De Pascale M.P.; De Santis C.; De Simone N.; Di Felice V.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobskiy S.; Krutkov Y.; Kvashnin A.N.; Leonov A.; Malakhov V.; Marcelli L.; Martucci M.; Mayorov A.G.; Menn W.; Merge M.; Mikhailov V.V.; Mocchiutti E.; Monaco A.; Mori N.; Munini R.; Osteria G.; Palma F.; Papini P.; Pearce M.; Picozza P.; Pizzolotto C.; Ricci M.; Ricciarini S.B.; Sarkar R.; Simon M.; Scotti V.; Sparvoli R.; Spillantini P.; Stozhkov Y.I.; Vacchi A.; Vannuccini E.; Vasilyev G.; Voronov S.A.; Yurkin Y.T.; Zampa G.; Zampa N.; Zverev V.G. (literal)
Pagina inizio
  • 273 (literal)
Pagina fine
  • 275 (literal)
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  • http://www.scopus.com/inward/record.url?eid=2-s2.0-84898001785&partnerID=q2rCbXpz (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 742 (literal)
Rivista
Note
  • Scopu (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence, Italy; INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy; University of Naples federico II, Department of Physics, I-80126 Naples, Italy; INFN, Sezione di Naples, I-80126 Naples, Italy; Lebedev Physical Institute, RU-119991, Moscow, Russian Federation; University of Bari, Department of Physics, I-70126 Bari, Italy; INFN, Sezione di Bari, I-70126 Bari, Italy; INFN, Sezione di Trieste, I-34149 Trieste, Italy; Ioffe Physical Technical Institute, RU-194021 St. Petersburg, Russian Federation; KTH, Department of Physics, AlbaNova University Centre, SE-10691 Stockholm, Sweden; Oskar Klein Centre for Cosmoparticle Physics, Sweden; INFN, Sezione di Rome Tor Vergata, I-00133 Rome, Italy; RIKEN, Advanced Science Institute, Wako-shi, Saitama, Japan; IFAC, I-50019 Sesto Fiorentino, Florence, Italy; University of Rome tor Vergata, Department of Physics, I-00133 Rome, Italy; University of Trieste, Department of Physics, I-34147 Trieste, Italy; NRNU MEPhI, RU-115409 Moscow, Russian Federation; INFN, Laboratori Nazionali di Frascati, Via Enrico Fermi 40, I-00044 Frascati, Italy; Universitat Siegen, Department of Physics, D-57068 Siegen, Germany; INFN, Sezione di Perugia, I-06123 Perugia, Italy; Agenzia Spaziale Italiana (ASI), Science Data Center, I-00044 Frascati, Italy (literal)
Titolo
  • Measurement of hydrogen and helium isotopes flux in galactic cosmic rays with the PAMELA experiment (literal)
Abstract
  • PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature, with particular focus on the antimatter component. The detector consists of a permanent magnet spectrometer core to provide rigidity and charge sign information, a Time-of-Flight system for velocity and charge information, a Silicon-Tungsten calorimeter and a Neutron detector for lepton/hadron identification. The velocity and rigidity information allow the identification of different isotopes for Z=1 and Z=2 particles in the energy range 100 MeV/n to 1 GeV/n. In this work we will present the PAMELA results on the H and He isotope fluxes based on the data collected during the 23rd solar minimum from 2006 to 2007. Such fluxes carry relevant information helpful in constraining parameters in galactic cosmic rays propagation models complementary to those obtained from other secondary to primary measurements such as the boron-to-carbon ratio. © 2013 Elsevier B.V. (literal)
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