A Study of Solar Energetic Particle Events of Cycle 23

Details A Study of Solar Energetic Particle Events of Cycle 23 A Study of Solar Energetic Particle Events of Cycle 23

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh23c..01c&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH23C-01

Physics

2101 Coronal Mass Ejections (7513), 7514 Energetic Particles (2114), 7534 Radio Emissions

Scientific paper

We examine the properties and associations of more than 200 solar proton events that extended above 25 MeV and occurred in the years 1997 through 2006. The properties include early peak intensities of e, H, He, O, and Fe, each at two different energies. The data are obtained from instruments on the IMP-8, SOHO, Wind, and ACE spacecraft. Solar event associations are made for as many events as possible and corresponding solar parameters are determined. These include Coronal Mass Ejection (CME) and flare properties and radio emissions from the metric through kilometric wavelength range. The events are divided into 5 major groups based on the relative abundances and particle profiles. Examples of events and basic correlations are illustrated. Tables containing our results will be made available via the internet.

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