Table 5: Best-fit model line fluxes at Earth in units of 10^-13 erg cm^-2 s^-1 for the high state ( upper section) and low state ( lower section) of  Vel. A comparison with observations, and the relative contributions from the three CIE components (1, 2, 3) and the photo-ionized component (4) are also listed.

(Å)	Ion	Flux		Contribution (%)
				1	2	3	4
1.87	Fe  -K	2.7	1.0	100	0	0	0
3.02	Ca  XX	0.05	-	100	0	0	0
3.18	Ca  XIX	0.86	0.93	89	11	0	0
3.73	Ar  XVIII	0.23	-	100	0	0	0
3.95	Ar  XVII	1.3	1.31	77	23	0	0
4.73	S  XVI	1.6	0.94	97	3	0	0
5.05	S  XV	5.9	1.08	41	59	0	0
5.68	Si  XIII	0.95	0.63	11	89	0	0
6.18	Si  XIV	2.	0.93	61	39	0	0
6.68	Si  XIII	8.0	1.15	8	92	0	0
8.42	Mg  XII	3.1	0.65	7	93	0	0
9.23	Mg  XI	2.2	1.27	1	95	4	0
10.24	Ne  X	0.62	0.77	2	95	3	0
12.13	Ne  X	1.1	1.14	0	91	9	0
13.60	Ne  IX	0.60	1.33	0	12	75	13
15.01	Fe  XVII	0.23	0.96	0	42	58	0
33.74	C  VI	0.35	0.83	0	0	0	100
13.60	Ne  IX	0.90	1.26	0	0	92	8
15.01	Fe  XVII	0.29	0.69	0	0	100	0
18.97	O  VIII	0.38	0.47	0	0	72	28
21.80	O  VII	0.22	1.10	0	0	11	89
33.74	C  VI	0.21	1.33	0	0	0	100