Spectroscopic Diagnostics for the N III Ion

Physics

Scientific paper

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Scientific paper

Spectroscopic diagnostics for the N iii ion have been studied using an atomic model including the first eleven energy levels and taking account of various physical processes. New calculations for the line emissivities as a function of electron density and temperature have been carried out. Density-sensitive and temperature-sensitive line emissivity ratios are presented and their diagnostic applications to the solar atmosphere are discussed with the help of available observations.

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