Abundances of Neon Isotopes in the Galactic Cosmic Rays (GCR) Measured by the Cosmic Ray Isotope Spectrometer (CRIS) on ACE

Details Abundances of Neon Isotopes in the Galactic Cosmic Rays (GCR) Measured by the Cosmic Ray Isotope Spectrometer (CRIS) on ACE Abundances of Neon Isotopes in the Galactic Cosmic Rays (GCR) Measured by the Cosmic Ray Isotope Spectrometer (CRIS) on ACE

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..aprw16005b&link_type=abstract

American Physical Society, April Meeting, April 29-May 2, 2000 Long Beach, CA, abstract #W16.005

Physics

Scientific paper

Neon isotopic abundances in the GCRs have been obtained using data from the CRIS experiment on ACE for the energy range 80-270 MeV/nuc. These abundance measurements and derived source abundances using a leaky box propagation model will be presented. Ne isotopic abundances in the anomalous cosmic rays (ACR) measured by the ACE-SIS experiment differ from those in the GCRs, indicating that either the GCR 22Ne has a different source than most GCRs (e.g. WR stars) or that the composition of the VLISM sampled by the ACR is different than the larger interstellar volume from which GCRs are accelerated.

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