Spectroscopic measurements of solar wind generation

Details Spectroscopic measurements of solar wind generation Spectroscopic measurements of solar wind generation

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280..47k&link_type=abstract

In JPL Solar Wind Five p 47-60 (SEE N84-13067 03-92)

Other

8

High Resolution, Plasma Generators, Solar Corona, Solar Wind, Spectroscopic Analysis, Electron Energy, Energy Transfer, Magnetic Fields, Magnetohydrodynamic Waves, Mathematical Models, Velocity Distribution

Scientific paper

Spectroscopically observable quantities are described which are sensitive to the primary plasma parameters of the solar wind's source region. The method is discussed in which those observable quantities are used as constraints in the construction of empirical models of various coronal structures. Simulated observations are used to examine the fractional contributions to observed spectral intensities from coronal structures of interest which co-exist with other coronal structures along simulated lines-of-sight. The sensitivity of spectroscopic observables to the physical parameters within each of those structures is discussed.

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