Elemental Composition and Energy Spectra of GCRs Measured by the Cosmic Ray Isotope Spectrometer (CRIS) on ACE at Solar Minimum

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We have measured the elemental abundances and energy spectra of galactic cosmic-ray nuclei using the CRIS instrument on the ACE spacecraft. The observations were made during a period of minimum solar activity between August 1997 and April 1998. Abundances and energy spectra for nuclei with charge from Z=5 to Z=28 and incident energies between 50 and 400 MeV/nucleon will be presented. These abundances will be compared to measurements made by other experiments performed during solar minima. A leaky-box propagation model has been used to derive elemental source abundances from the CRIS measurements.

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