Temporal variations of solar flare nucleon abundances and their implications for acceleration and coronal propagation

Details Temporal variations of solar flare nucleon abundances and their implications for acceleration and coronal propagation Temporal variations of solar flare nucleon abundances and their implications for acceleration and coronal propagation

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4...31m&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

Physics

Abundance, Nucleons, Particle Acceleration, Solar Corona, Solar Flares, Radio Bursts, Shock Wave Propagation

Scientific paper

The authors show that in poorly-connected solar particle events the
≡1 MeV/nucleon He/H, O/He and Fe/He ratios and their random
fluctuations are uncorrelated with flare site location.

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