Physics
Scientific paper
Nov 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...9916367e&link_type=abstract
Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States
Physics
Solar Wind, Electron Energy, Coronal Holes, Chromosphere, Coronas, Solar Atmosphere, Plasmas (Physics), Acceleration (Physics)
Scientific paper
Flow speeds derived in recent years from chromospheric/transition region and coronal observations suggest that the solar wind acceleration process might start at heights in the solar atmosphere much lower than previously imagined. The goal of the proposed investigation was to study atmospheric outflows in coronal hole regions from the chromosphere into the corona using observational and theoretical approaches. In addition to outflows, other plasma properties such as electron densities, and electron and ion temperatures were also included in the study. To investigate these plasma properties in the inner corona is important as they play a crucial role in placing limits on possible coronal heating and solar wind acceleration mechanisms.
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