Ionization states of heavy elements observed in the 1974 May 14-15 anomalous solar particle event

Details Ionization states of heavy elements observed in the 1974 May 14-15 anomalous solar particle event Ionization states of heavy elements observed in the 1974 May 14-15 anomalous solar particle event

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8117973m&link_type=abstract

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Physics

Heavy Ions, Solar Corpuscular Radiation, Solar Flares, Solar Physics, Explorer 50 Satellite, Ion Cyclotron Radiation, Iron, Plasma Heating

Scientific paper

The charge states of heavy ions accelerated in the (3)He-Fe rich solar particle event of 1974 May 14-15 are determined using data from the Interplanetary Monitoring Platform-8. In addition to Fe(+11,12) both 0(+5) and Fe(+16,17,18) are also present suggesting variations in coronal temperatures over a range from approximately 400,000 to 5,000,000 K. The presence of 0(+5) and Fe(+16-18) may be explained by a resonant plasma heating mechanism proposed to account for the enhancements of (3)He and Fe.

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