Highly Ionized sodium X-ray line emission from the solar corona and the abundance of sodium

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Table 2:

Selected Na IX satellite lines excited by dielectronic recombination: data from the Cowan HFR code.
Wavelength (Å)^a	Line label^b	Transition	$B_{\rm sat}$ (s^-1)^c	$E_{\rm sat}$ (Ry)
11.043	d15	$\rm 1s^2 3p~ ^2P_{1/2} {-} 1{\rm s} 2p 3p~ (^1P)~^2D_{3/2}$	3.33(13)	73.5
11.044	d13	$\rm 1s^2 3p~ ^2P_{3/2} {-} 1{\rm s} 2p 3p~ (^1P)~^2D_{5/2}$	5.77(13)	73.5
11.077^d	s	$\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s} 2p^2~ (^3S)~^2P_{3/2}$	4.64(12)	60.0
11.078^d	t	$\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~(^3S)~^2P_{1/2}$	2.90(12)	60.0
11.105	n	$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2S_{1/2}$	3.11(12)	60.6
11.108	m	$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2S_{1/2}$	8.19(12)	60.6
11.152^d	q	$\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~(^1S)~^2P_{3/2}$	1.66(13)	60.6
11.155^d	r	$\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~(^1S)~^2P_{1/2}$	9.61(12)	60.6
11.165	b	$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2P_{3/2}$	3.28(11)	60.6
11.168	d	$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2P_{1/2}$	7.12(10)	60.6
11.168	a	$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2P_{3/2}$	2.13(12)	60.6
11.171	c	$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2P_{1/2}$	3.25(10)	60.6
11.188	k	$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2D_{3/2}$	2.31(13)	60.6
11.191	j	$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2D_{5/2}$	3.70(13)	60.6
11.192	l	$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2D_{3/2}$	1.90(12)	60.6
11.286	e	$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^4P_{5/2}$	1.74(10)	60.6
11.298^d	u	$\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s} 2p^2~ (^3S)^4P_{3/2}$	3.45(9)	60.0
11.300^d	v	$\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~ (^3S)^4P_{1/2}$	6.64(8)	60.0

Notes. ^(a) Wavelengths from Cowan code + 0.001 Å; ^(b) Notation of Gabriel (1972); Bely-Dubau et al. (1979); ^(c) Numbers in parentheses are powers of ten; ^(d) Lines also formed by inner-shell excitation.

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