Expected intensities of solar forbidden lines emitted from 2p(k) (k = 2, 3, 4) configurations

Details Expected intensities of solar forbidden lines emitted from 2p(k) (k = 2, 3, 4) configurations Expected intensities of solar forbidden lines emitted from 2p(k) (k = 2, 3, 4) configurations

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...85...41k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 85, May 1983, p. 41-51.

Physics

7

Forbidden Transitions, Solar Corona, Solar Spectra, Transition Probabilities, Ultraviolet Spectra, Atomic Energy Levels, Atomic Excitations, Emission Spectra, Extreme Ultraviolet Radiation, Ground State, Ions, Populations, Spectral Line Width

Scientific paper

Predicted intensities of all significant transitions within the ground configurations of six-, seven-, and eight-electron ions are tabulated for solar conditions, on a common scale. Some applications of the table entries to line identification and emission measure analysis are presented, including proposed Mg VI classifications for the coronal lines 3488.5 Å and 3502.5 Å.

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