Investigation of the Large Scale Evolution and Topology of Coronal Mass Ejections in the Solar Wind

Details Investigation of the Large Scale Evolution and Topology of Coronal Mass Ejections in the Solar Wind Investigation of the Large Scale Evolution and Topology of Coronal Mass Ejections in the Solar Wind

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...0010917r&link_type=abstract

Technical Report, Rept-21

Physics

Coronal Mass Ejection, Advanced Composition Explorer, Solar Wind, Topology, Plasmas (Physics), Magnetohydrodynamics, Geomagnetism, Magnetic Flux, Low Density Research, Three Dimensional Models, Solar Corona, Data Integration

Scientific paper

This investigation is concerned with the large-scale evolution and topology of Coronal Mass Ejections (CMEs) in the solar wind. During this reporting period we have analyzed a series of low density intervals in the ACE (Advanced Composition Explorer) plasma data set that bear many similarities to CMEs. We have begun a series of 3D, MHD (Magnetohydrodynamics) coronal models to probe potential causes of these events. We also edited two manuscripts concerning the properties of CMEs in the solar wind. One was re-submitted to the Journal of Geophysical Research.

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