Physics
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh11a0371m&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #SH11A-0371
Physics
2164 Solar Wind Plasma, 7509 Corona, 7549 Ultraviolet Emissions, 7835 Magnetic Reconnection (2723, 7526), 7867 Wave/Particle Interactions (2483, 6984)
Scientific paper
The Solar Wind Focused Science Topic (FST) team was created to apply a combination of theoretical studies, numerical simulations, and observations to the understanding of how the fast and slow solar wind are heated and accelerated. Four proposals were selected for this FST team. They will investigate the role of energy sources and kinetic mechanisms responsible for the heating and acceleration of the solar wind. In particular, the FST team will examine magnetic reconnection 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, will be used to put firm constraints on the models. The work of the Solar Wind FST team is in its initial stages. The organization, planning, and findings resulting from the first FST team meeting will be reported.
Bhattacharjee Anirban
Cranmer Steven R.
Doschek George A.
Forbes Terry G.
Isenberg Philip A.
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