Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment (Articolo in rivista)

Type
Label
  • Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with 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
  • 10.1088/0004-637X/770/1/2 (literal)
Alternative label
  • Adriani, O., Barbarino, G.C., Bazilevskaya, G., Castellini, G., Ricciarini S.B., ET AL. (2013)
    Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment
    in The Astrophysical journal
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Adriani, O., Barbarino, G.C., Bazilevskaya, G., Castellini, G., Ricciarini S.B., ET AL. (literal)
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  • 770 (literal)
Rivista
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  • 1 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • Department of Physics, University of Florence, I-50019 Sesto Fiorentino, Florence, Italy; INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy; Department of Physics, University of Naples Federico II, I-80126 Naples, Italy INFN, Sezione di Naples, I-80126 Naples, Italy; Lebedev Physical Institute, RU, 119991 Moscow, Russian Federation; \"Nello Carrara\" Institute of Applied Physics (IFAC) of the National Research Council (CNR), Florence, Italy (literal)
Titolo
  • Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment (literal)
Abstract
  • The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hydrogen and between 100 and 900 MeV/n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C. © 2013. The American Astronomical Society. All rights reserved. (literal)
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