Geoeffective CMEs and Energetic Particles: The Influence of Ambient Solar Wind

Details Geoeffective CMEs and Energetic Particles: The Influence of Ambient Solar Wind Geoeffective CMEs and Energetic Particles: The Influence of Ambient Solar Wind

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....10821l&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #10821

Physics

Scientific paper

Geoeffective coronal mass ejections (CMEs) are often associated with energetic storm particles (ESP), which are accelerated locally at the shock front. A recent study showed that the CME transit time, estimated from the ESP onset, is correlated with the geomagnetic storm strength, but the ESP shock peak properties were not as useful. The study did not, however, take into account the effect of the ambient plasma properties to the ESP acceleration and transport. We study the local solar wind conditions on 16 ESP events, and estimate their influence to the prediction of the CME and storm properties.

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