Mapping the Solar Wind from its Source Region into the Outer Corona

Details Mapping the Solar Wind from its Source Region into the Outer Corona Mapping the Solar Wind from its Source Region into the Outer Corona

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998sao..reptq....e&link_type=abstract

Technical Report, NASA/CR-1998-208346; NAS 1.26:208346

Physics

Mapping, Solar Wind, Plasmas (Physics), Coronas, X Rays, Scintillation, Line Spectra, Heating, Brightness, Acceleration (Physics)

Scientific paper

Knowledge of the radial variation of the plasma conditions in the coronal source region of the solar wind is essential to exploring coronal heating and solar wind acceleration mechanisms. The goal of the present proposal is to determine as many plasma parameters in that region as possible by coordinating different observational techniques, such as Interplanetary Scintillation Observations, spectral line intensity observations, polarization brightness measurements and X-ray observations. The inferred plasma parameters are then used to constrain solar wind models.

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