On the EUV Line Diagnostics From N III Solar Ion

Details On the EUV Line Diagnostics From N III Solar Ion On the EUV Line Diagnostics From N III Solar Ion

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997basi...25..247g&link_type=abstract

Bulletin of the Astronomical Society of India, vol. 25, p. 247

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Applications

Extreme Ultraviolet Radiation, Solar Atmosphere, Line Spectra, Nitrogen Plasma, Plasma Diagnostics, Emissivity, Electron Density (Concentration), Electron Energy, Atomic Energy Levels

Scientific paper

We present new calculations for N III ion for diagnostics of solar plasma. The atomic model comprising the first 15 energy levels is considered for evaluating the line emissivities as a function of electron density and temperature, taking account of various physical processes. EUV line ratios, hitherto unexplored for diagnostic study, from this ion are presented as a function of electron density at its temperature of peak ionic concentration and their diagnostic applications in the solar atmosphere are discussed.

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