Recommended programs for galactic cosmic rays (less than 1 TeV/nucleon) for the years 2000-2010

Details Recommended programs for galactic cosmic rays (less than 1 TeV/nucleon) for the years 2000-2010 Recommended programs for galactic cosmic rays (less than 1 TeV/nucleon) for the years 2000-2010

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203..231b&link_type=abstract

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

Computer Science

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Balloon Sounding, Galactic Cosmic Rays, Galactic Evolution, Nasa Space Programs, Abundance, Energy Spectra, Heavy Nuclei, Nuclear Reactions, Particle Accelerators, Solar System

Scientific paper

The discussions and recommendations from the group meeting on galactic cosmic rays (less than 1 TeV/nucleon), part of the workshop on 'The NASA Cosmic Ray Program for the 1990's and Beyond', are presented. Attention is focused on the importance of continued laboratory investigations, particularly cross section measurements at the Bevalac, and continued support for a strong ballooning program. The broad science goals addressed are: to study the origin and evolution of galactic matter, and to investigate acceleration, transport, and time scales of galactic cosmic rays.

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