Solar He-3-rich events observed on ISEE-3

Details Solar He-3-rich events observed on ISEE-3 Solar He-3-rich events observed on ISEE-3

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4...48r&link_type=abstract

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

Physics

Abundance, International Sun Earth Explorer 3, Solar Activity, Solar Cosmic Rays, Solar Flares, Anisotropy, Helium, Solar Magnetic Field

Scientific paper

A scan has been made of ISEE-3 data for all events with He-3/He-4 between 0.20 and 1.3 MeV/nucl. The 67 events found show some evidence of 27-day recurrence. Larger events show both velocity dispersion and magneic field-aligned arrival from the solar direction. At least one third of the events are preceded by increases in about 300 keV electrons, although several larger events show no electron increases. Spike events also exist suggesting nearly scatter-free propagation of He-3 from well-connected events.

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