Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976asaer..14...24d&link_type=abstract
Astronautics and Aeronautics, vol. 14, July-Aug. 1976, p. 24-30.
Astronomy and Astrophysics
Astronomy
High Temperature Plasmas, Plasma Diagnostics, Solar Atmosphere, Spectrum Analysis, Anisotropic Fluids, Electron Density (Concentration), Electron Energy, Far Ultraviolet Radiation, Ion Density (Concentration), Ion Temperature, Laser Plasmas, Light (Visible Radiation), Solar Flares, Solar Wind, Turbulent Flow, X Ray Spectroscopy
Scientific paper
In recent years, high-resolution spectroscopy in the X-ray, extreme-ultraviolet, ultraviolet, and visible spectral regions has found increasing application for the study of conditions in solar plasmas. The use of spectroscopic techniques in the X-ray and extreme-ultraviolet spectral regions to determine such physical quantities as electron and ion temperature, electron and ion density, turbulence or anisotropic motions, and the departure of the ionic species from kinetic equilibrium in solar and laboratory plasmas is discussed. Solar-flare spectra are compared to the spectra of active solar regions.
Doschek George A.
Feldman Uri
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