Precision Measurements of Solar Energetic Particle Elemental Composition

Details Precision Measurements of Solar Energetic Particle Elemental Composition Precision Measurements of Solar Energetic Particle Elemental Composition

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..213b&link_type=abstract

Proceedings from the 19th International Cosmic Ray Conference, Volume 4 (SH Sessions), p.213

Physics

Scientific paper

Using data from the Cosmic Ray Subsystem aboard the Voyager 1 and 2 spacecraft (Stone et al., 1977), the authors have determined solar energetic particle abundances or upper limits for all elements with 3 ≤ Z ≤ 30 from a combined set of 10 solar flares during the 1977 - 1982 time period. Statistically meaningful abundances have been determined for the first time for several rare elements including P, Cl, K, Ti and Mn, while the precision of the mean abundances for the more abundant elements has been improved by typically a factor of ≡3 over previously reported values.

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