Elemental composition of low energy Galactic cosmic rays

Details Elemental composition of low energy Galactic cosmic rays Elemental composition of low energy Galactic cosmic rays

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aipc..183..388f&link_type=abstract

IN: Cosmic abundances of matter; Proceedings of the AIP Conference, Minneapolis, MN, Sept. 7-9, 1988 AIP Conference Proceedings,

Physics

1

Chemical Composition, Chemical Elements, Galactic Cosmic Rays, Milky Way Galaxy, Nitrogen, Oxygen, Telescopes, Voyager 2 Spacecraft

Scientific paper

This paper describes new measurements (at about 100 MeV/n) of elemental ratios in cosmic rays, made from Voyager 2 at about 22.5 AU. These data are characterized by a very low level of solar modulation, which results from the combination of the 1986-1987 solar minimum period and the large heliocentric distance. The data were obtained from one of the two HET telescopes on board Voyager 2, collected during 1986 and 1987; the charges were derived from a double dE/dx vs E analysis. The results on the secondary/primary elemental ratios are presented along with previous results obtained at 1 AU by IMP-8 and ISEE-3.

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