ACE/EPAM Energetic Particle Signatures during the October/November 2003 Interplanetary Coronal Mass Ejection Events

Details ACE/EPAM Energetic Particle Signatures during the October/November 2003 Interplanetary Coronal Mass Ejection Events ACE/EPAM Energetic Particle Signatures during the October/November 2003 Interplanetary Coronal Mass Ejection Events

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..176m&link_type=abstract

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Astronomy and Astrophysics

Astrophysics

Coronal Mass Ejection, Particle Emission, Solar Wind

Scientific paper

Solar energetic particles are utilized as diagnostic tracers of the large-scale structure and topology of the Interplanetary Magnetic Field embedded within two Interplanetary Coronal Mass Ejections detected in late October and early November 2003 at 1 AU by the ACE spacecraft. Two candidate scenarios to account for the observations in terms of open and closed magnetic field configurations are examined. We also use ACE/EPAM observations to reassess the boundaries of the ICMEs with respect to those previously proposed.

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