The isotopic composition of cosmic ray nuclei beyond the iron peak

Details The isotopic composition of cosmic ray nuclei beyond the iron peak The isotopic composition of cosmic ray nuclei beyond the iron peak

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203..268m&link_type=abstract

IN: Particle astrophysics - The NASA cosmic ray program for the 1990s and beyond (A92-20526 06-93). New York, American Institute

Physics

Nuclear Physics

Cosmic Rays, Iron, Isotopes, Nuclear Astrophysics, Nuclei (Nuclear Physics), Abundance, Mass Distribution, Optical Fibers, Particle Acceleration, Radiation Detectors

Scientific paper

Isotope measurements of cosmic ray nuclei beyond the Fe peak are considered, using the charge region from Z = 29 to Z about 40 as an example. Such studies can address a number of important questions that bear on cosmic ray origin, acceleration, and propagation. One possible approach for measuring isotopes with Z equal to or greater than 30 is based on large-area arrays of silicon solid state detectors combined with scintillating optical fiber trajectory detectors.

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