Published 2003
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New Measurement of the Li, Be, an B Isotopes as a Test of Cosmic Ray Transport Models
Abstract
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-measured production cross-sections for these isotopes help to improve our understanding of galactic cosmic ray propagation models. The Cosmic Ray Isotope 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.
Additional Information
Copyright Universal Academy Press Inc. This work was supported by NASA at NASA/GSFC, California Inst. of Tech., Jet Propulsion Laboratory, and Washington University.Attached Files
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Additional details
- Eprint ID
- 56385
- Resolver ID
- CaltechAUTHORS:20150406-135715114
- NASA
- California Institute of Technology
- JPL
- Washington University
- Created
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2015-04-15Created from EPrint's datestamp field
- Updated
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2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2003-20