Computer Science
Scientific paper
Oct 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....1..310g&link_type=abstract
In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 1. (A81-12386 02-93) T
Computer Science
1
Abundance, Chemical Elements, Cosmic Rays, Energy Spectra, Mass Ratios, Satellite Observation, Boron, Carbon, Galactic Radiation, Imp, Iron, Kinetic Energy, Manganese, Nitrogen, Oxygen, Samarium, Solar Activity Effects
Scientific paper
The secondary to primary ratios B/C, N/O and (Sc-Mn)/Fe in the galactic cosmic rays have been measured in the overall energy interval 30-180 MeV/n with the University of Chicago cosmic ray telescope on board the satellite IMP-8 during the period 1974-1978. These results, together with the values of the same ratios measured at higher energies, have been compared to the results of cosmic ray propagation calculations using different pathlength distributions (PLD) and different levels of solar modulation, in order to select a single set of parameters consistent with all the measured ratios.
Garcia-Munoz Manuel
Margolis Steven H.
Simpson André J.
Wefel John P.
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