A spectroscopic analysis of the most polarizing atomic lines of the second solar spectrum

Free Access

Table 3:

Lines of Table 2 produced by subordinate transitions, and corresponding resonance lines.
Subordinate trans.				Resonant trans.
El.	$\lambda$	Q/I	type	$\lambda$	Q/I	type
	(Å)	(%)		(Å)	(%)
H I	4340.475	0.12	W	1216 [Ly $_{\alpha }$ ]	outside
	6562.808	0.109	S	1216 [Ly $_{\alpha }$ ]	atlas range
Mg I	5528.418	0.052	W	2852	outside
	4703.003	0.050	W	2852	atlas range
Ca II	3179.342	0.35	W	3933.682	0.90	M1
Fe I	6024.068	0.05	S	4045.825	0.390	M1
Cu I	5218.209	0.052	S	3247.540	0.93	M0
Ba II	4130.657	0.28	S	4554.036	0.65	MS

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.