The Solar Cycle Variability of Solar Energetic Particle Composition

Details The Solar Cycle Variability of Solar Energetic Particle Composition The Solar Cycle Variability of Solar Energetic Particle Composition

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3237l&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Solar particle isotopic composition varies greatly from event to event, apparently due to mass fractionation during particle acceleration and/or transport. We examine whether the amount of this variability changes during the solar cycle and find a strong indication of less isotopic compositional variability at solar maximum than during less active phases. There also seems to be a similiar but weaker association using elemental abundances. The underlying cause of the variability and reasons why it might change over the solar cycle are yet to be determined.

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