The composition of corotating energetic particle streams

Details The composition of corotating energetic particle streams The composition of corotating energetic particle streams

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7821039m&link_type=abstract

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Computer Science

Concentration (Composition), Nucleons, Particles, Rotating Plasmas, Helium, Interplanetary Medium, Ions, Solar Flares, Solar Wind

Scientific paper

The relative abundances of 1.5 to 23 MeV/nucleon ions in corotating nucleon streams were compared with ion abundances in particle events associated with solar flares and with solar and solar wind abundances. He/O and C/O ratios were found to be a factor of the order two to three times greater in corotating streams than in flare associated events. The distribution of H/He ratios in corotating streams was found to be much narrower and of lower average value than in flare associated events. H/He in corotating energetic particle streams compared favorably both in lack of variability and numerical value to H/He in high speed solar wind plasma streams. This comparison suggested that the source population for the corotating energetic particles was the solar wind.

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