Expected intensities of solar forbidden lines emitted from 2p
k
(k = 2, 3, 4) configurations |
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Authors: | S O Kastner |
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Institution: | 1. Laboratory for Astronomy and Solar Physics, NASA-Goddard Space Flight Center, 20771, Greenbelt, MD, U.S.A.
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Abstract: | 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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