Physics
Scientific paper
Feb 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000stin...0023158r&link_type=abstract
Technical Report, SciberNet, Inc. San Diego, CA United States
Physics
Stellar Evolution, Topology, Coronal Mass Ejection, Solar Corona, Solar Wind, Magnetohydrodynamics, Simulation, Thermalization (Energy Absorption)
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 focused on several aspects of CME properties, their identification and their evolution in the solar wind. The work included both analysis of Ulysses and ACE observations as well as fluid and magnetohydrodynamic simulations. In addition, we analyzed a series of "density holes" observed in the solar wind, that bear many similarities with CMEs. Finally, this work was communicated to the scientific community at three meetings and has led to three scientific papers that are in various stages of review.
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