Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh13b1528m&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SH13B-1528
Physics
2164 Solar Wind Plasma, 7509 Corona, 7549 Ultraviolet Emissions, 7835 Magnetic Reconnection (2723, 7526), 7867 Wave/Particle Interactions (2483, 6984)
Scientific paper
We present a summary of the research conducted by the members of the 2006 LWS TR&T Solar Wind Focused Science Topic (FST) Team on the physical processes that heat and accelerate the solar wind. The Team applied a combination of theoretical studies, numerical simulations, and observations for their investigation of the role of energy sources and kinetic mechanisms responsible for the heating and acceleration of the solar wind. In particular, the FST Team examined magnetic reconnection, waves, and turbulence as possible heating mechanisms. Plasma properties and their evolution over the solar cycle, determined from the analysis of remote and in situ measurements of solar wind source regions and streams, are being used to constrain the models. The consistency of candidate theoretical models with existing observational data for the solar wind will be discussed.
LWS Tr&T Solar Wind Fst Team
Miralles Mari Paz
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