NASA NTRS · 19730059833
Theoretical intensity ratios for some Fe XIII coronal lines.
Abstract
Using cross section values for collisional excitation by protons recently calculated by Landman (1973), theoretical values for the relative intensities of the Fe XIII 10747-, 10798-, and 3388-A lines are determined as functions of electron density. The obtained results are compared with those of Chevalier and Lambert (1969).
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Finn, G. D., Landman, D. A.. 1973-06-01. Theoretical intensity ratios for some Fe XIII coronal lines.. https://ntrs.nasa.gov/citations/19730059833
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