New Measurements of the Li, Be, and bIsotopes as a Test of Cosmic Ray Transport Models

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Scientific paper

Precise measurements of predominantly secondary cosmic-ray Li, Be, and btogether with current well-measured production cross-sections for these isotop es help to improve our understanding of galactic cosmic ray propagation models. The Cosmic Ray Isotop e spectrometer (CRIS) on ACE has been measuring isotopic composition of cosmic rays since 1997 with high statistical precision. We present the isotopic abundances from CRIS and discuss these observations in the context of cosmic-ray transport models and previous cosmic-ray measurements.

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