Elemental Abundances for 3 <= Z <= 30 Galactic Cosmic Ray Nuclei Measured by the Cosmic Ray Isotope Spectrometer on ACE

Details Elemental Abundances for 3 <= Z <= 30 Galactic Cosmic Ray Nuclei Measured by the Cosmic Ray Isotope Spectrometer on ACE Elemental Abundances for 3 <= Z <= 30 Galactic Cosmic Ray Nuclei Measured by the Cosmic Ray Isotope Spectrometer on ACE

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..apr..c807l&link_type=abstract

American Physical Society, APS/AAPT Joint April Meeting, April 18-21, 1998 Columbus, Ohio, abstract #C8.07

Physics

Scientific paper

The Cosmic Ray Isotope Spectrometer (CRIS) on ACE is composed of four stacks of silicon detectors which provide multiple dE/dx and total energy measurements, and a scintillating fiber hodoscope which measures trajectory and enables us to make angle corrections to the silicon detector signals for stopping cosmic ray nuclei. Data collected in-flight have been used to determine the elemental abundances of nuclei with 3 <= Z <= 30 over the energy range 50 <= E <= 500 MeV/nuc. These data will be presented and compared with measurements from previous experiments.

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