SEPs and CMEs during cycle 23

Details SEPs and CMEs during cycle 23 SEPs and CMEs during cycle 23

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..475m&link_type=abstract

Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 475-477

Astronomy and Astrophysics

Astronomy

Acceleration Of Particles, Sun: Coronal Mass Ejections (Cmes), Sun: Particle Emission

Scientific paper

We present a study of solar energetic particles (SEPs) in association with coronal mass ejections (CMEs) and type II radio bursts. The particle and CME observations cover the years 1996-2007. We find that heavy-ion events in association with type II bursts and proton events are produced in more western and most energetic CMEs. In addition, the source distribution of type II associated proton events with heavy ions reminds the source distribution expected for events with flare particles. Therefore, the estimation of relative contributions by flares and shocks in SEP events and separation of suggested different particle acceleration models is complicated.

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