A Study of Solar Energetic Particle Events and Coronal Mass Ejections Using SOHO Data

Details A Study of Solar Energetic Particle Events and Coronal Mass Ejections Using SOHO Data A Study of Solar Energetic Particle Events and Coronal Mass Ejections Using SOHO Data

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004padeu..14...57f&link_type=abstract

In: Proceedings of the British-Hungarian N+N Workshop for Young Researchers On Computer processing and use of satellite data in

Astronomy and Astrophysics

Astrophysics

Scientific paper

The relation of coronal mass ejections (CMEs) and solar energetic particle events (SEPs) is a field where our understanding of the underlying physical processes has been subject to rapid changes recently. Two paradigms are still competing: the earlier one is that solar energetic particle events (SEPs) are triggered by flares. The recently more popular viewpoint is that from the two classes of SEPs, gradual events and impulsive events, only the latter are caused by flares, large spectacular gradual events are related to CMEs, and entirely unrelated to flares. Most recent observations seem to indicate that many events do not fit into this simplified scheme, and many combinations termed as hybrid events may exist. Here I present two typical SEPs, and then two new ``hybrid'' class SEPs are reviewed.

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