Physics
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998sao..reptt....e&link_type=abstract
Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States
Physics
Chromosphere, Coronal Holes, Coronas, Plasmas (Physics), Solar Atmosphere, Solar Wind, Atmospheric Models, Dynamic Characteristics, Estimates
Scientific paper
The dynamic behavior of the plasma in the chromosphere/transition region /inner corona is vital for the acceleration of the solar wind. With new theoretical descriptions of the solar atmosphere and corona, and the increased observational possibilities provided by the SOHO spacecraft, it is possible to conduct an integrated study of the solar atmosphere and corona using observational and theoretical approaches. Over the past few years a series of observational techniques have been used to estimate the solar wind densities, temperatures and flow speed in the inner corona. These estimates suggest that the solar wind has higher outflow speeds in the inner corona and lower densities than previously assumed. A comparison with densities derived from atmospheric models support these lower densities.
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