N III lines for solar diagnostics

Details N III lines for solar diagnostics N III lines for solar diagnostics

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....71l...5n&link_type=abstract

Astronomy and Astrophysics, vol. 71, no. 1-2, Jan. 1979, p. L5-L8.

Astronomy and Astrophysics

Astrophysics

86

Far Ultraviolet Radiation, Nitrogen Atoms, Solar Spectra, Spectroheliographs, Ultraviolet Spectra, Abundance, Boron, Gas Density, Gas Temperature, Iue, Line Spectra, Satellite Observation, Temperature Effects

Scientific paper

The EUV N III spectrum is discussed with reference to the interpretation of solar observations. Atomic data are presented which will also be useful in the investigation of other astronomical objects, such as for the N III 1749-A multiplet in IUE observations. From the ATM observation excitation temperatures are found which lie significantly below the temperature of maximum fractional abundance of N(2+).

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