The measurement of elemental abundances above 1 TeV/amu by a long duration flight of CRN

Details The measurement of elemental abundances above 1 TeV/amu by a long duration flight of CRN The measurement of elemental abundances above 1 TeV/amu by a long duration flight of CRN

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203..125s&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

Abundance, Galactic Cosmic Rays, Long Duration Space Flight, Nuclei (Nuclear Physics), Radiation Detectors, Particle Energy, Satellite-Borne Instruments, Spacelab Payloads

Scientific paper

The flight of the Cosmic Ray Nuclei detector (CRN), for a long duration of at least one year is proposed. The instrument has already flown successfully on the Spacelab-2 mission, using transition radiation detectors to provide individual elemental abundances to energies of 1 TeV/amu for Z between 4 and 30. The dynamic range of the instrument permits measurements to much higher energies if a longer exposure time can be facilitated. With a one-year flight, the number of particles collected would provide data to roughly 10 TeV/amu or beyond.

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