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ADRIANI, O; Barbarino, G C; BAZILEVSKAYA, G A; Bellotti, R; BOEZIO, M; Bogomolov, E A; BONGI, M; Bonvicini, V; Borisov, S; Bottai, S
The Astrophysical journal, 06/2013, Letnik: 770, Številka: 1Journal Article
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.
