Physics
Scientific paper
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.
Binns Robert W.
Christian Eric R.
Cummings Alan C.
George Samuel J.
Hink Paul L.
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