Table 5.

Xenon in Genesis AloS solar wind collectors released in four different laser ablation experiments. Analysis with zero rastered areas are weighted average of several blank analyses.

Sample, extract, method	Area (cm2)	Total 132Xe, 106 at.	132Xe = 1000								Fraction of SW		SW 132Xe retrieved 106 at/cm2
			136Xe	134Xe	131Xe	130Xe	129Xe	128Xe	126Xe	124Xe	84Kr/132Xe	132Xe
A-π/8(a)	0.00	0.01	3004 ± 151	3636 ± 173	<12374	1434 ± 91	10115 ± 280	857 ± 83	n.d.	n.d.	22.9	.100
	0.81	1.09	3021 ± 36	3736 ± 37	8167 ± 95	1603 ± 25	10440 ± 74	831 ± 19	41.8 ± 4.1	46.4 ± 4.8	10.4	.943	1.26
	0.72	0.98	2967 ± 47	3723 ± 50	8090 ± 145	1641 ± 38	10225 ± 86	811 ± 21	37.0 ± 4.6	54.0 ± 5.6	11.2	.889	1.22
	0.38	0.60	2995 ± 55	3731 ± 61	7859 ± 350	1577 ± 40	10315 ± 97	805 ± 30	39.5 ± 4.9	54.8 ± 8.0	12.1	.829	1.31
	0.052	0.07	2929 ± 135	3649 ± 150	8399 ± 520	1501 ± 93	10410 ± 125	782 ± 71	41 ± 17	50 ± 24	11.6	.863	1.13
A-π/8(b)	0.96	1.20	3029 ± 17	3653 ± 20	8574 ± 66	1621 ± 21	10393 ± 38	863 ± 9	45.7 ± 2.0	56.6 ± 3.0	9.78	.985	1.23
	3.82	4.31	3007 ± 9	3671 ± 11	8238 ± 17	1665 ± 6	10354 ± 19	839 ± 4	42.7 ± 1.1	46.8 ± 1.0	9.90	.976	1.10
	0.84	1.18	3046 ± 15	3754 ± 18	8419 ± 55	1649 ± 12	10377 ± 33	827 ± 8	41.8 ± 2.0	49.2 ± 2.8	11.4	.875	1.23
	0.32	0.43	3030 ± 56	3732 ± 31	8396 ± 84	1613 ± 19	10334 ± 59	872 ± 13	41.9 ± 3.0	50.9 ± 4.1	10.2	.956	1.28
A-π/4	0.00	0.03	3335 ± 410	3754 ± 300	<11423	1937 ± 230	10159 ± 740	791 ± 221	n.d.	n.d.	25.8	−0.093
	3.75	9.37	3070 ± 35	3737 ± 40	8112 ± 35	1601 ± 22	10055 ± 29	798 ± 9	35.7 ± 2.0	40.6 ± 2.1	19.3	0.340	0.85
	0.44	.500	3011 ± 45	3726 ± 50	8247 ± 93	1607 ± 27	10396 ± 110	818 ± 20	36.0 ± 6.1	46.1 ± 4.5	11.3	0.884	1.01
	0.78	1.02	3060 ± 43	3717 ± 50	8147 ± 48	1640 ± 37	10318 ± 94	796 ± 23	38.1 ± 5.4	54.7 ± 6.8	11.5	0.866	1.13
	0.15	0.20	3079 ± 81	3682 ± 73	8164 ± 108	1613 ± 59	10272 ± 167	830 ± 29	35.9 ± 5.9	51.7 ± 8.0	12.6	0.794	1.08
	0.24	0.26	3087 ± 55	3789 ± 71	8240 ± 98	1633 ± 50	10322 ± 137	833 ± 28	38.0 ± 5.2	45.2 ± 7.3	10.7	0.921	0.98
	0.72	0.87	3023 ± 50	3757 ± 49	8189 ± 62	1609 ± 25	10323 ± 94	814 ± 20	40.1 ± 4.0	50.1 ± 4.8	11.7	0.855	1.03
A-π	0.00	0.02	3203 ± 300	3675 ± 290	<10200	1501 ± 192	10330 ± 560	998 ± 294	n.d.	n.d.	18.3	0.041
	1.48	1.94	3016 ± 20	3678 ± 51	8184 ± 55	1628 ± 24	10323 ± 19	809 ± 16	40.3 ± 4.2	53.4 ± 1.8	10.5	0.933	1.22
	0.20	0.28	2913 ± 90	3650 ± 94	8408 ± 167	1592 ± 87	10252 ± 30	790 ± 53	48.2 ± 7.4	63.7 ± 9.2	12.4	0.808	1.18
	0.84	1.18	3015 ± 50	3759 ± 48	8268 ± 96	1649 ± 27	10491 ± 96	799 ± 23	39.2 ± 4.7	47.5 ± 4.9	11.3	0.881	1.23
	0.32	0.34	3045 ± 57	3762 ± 68	8438 ± 109	1684 ± 38	10493 ± 23	796 ± 25	44.8 ± 5.5	55.7 ± 6.9	10.0	0.966	1.05
	0.24	0.31	3081 ± 92	3771 ± 97	8436 ± 186	1585 ± 83	10322 ± 22	805 ± 46	42.7 ± 7.5	38.2 ± 9.8	10.5	0.936	1.24
	0.80	0.95	3045 ± 24	3780 ± 20	8116 ± 28	1585 ± 11	10268 ± 37	811 ± 8	36.5 ± 2.0	43.4 ± 1.8	11.0	0.903	1.07
Atmospheric Xe Basford et al. (1973)			3294 (4)	3879 ± 6	7890 ± 11	1513.6 ± 1.2	9832 ± 12	713.6±.9	33.00±.17	35.37±.11

Notes: Stated errors are 1σ. Errors for gas concentrations and elemental ratios are 5–7% based on the scatter observed in series of air standards measured prior and after each experiment. (⁸⁴Kr/¹³²Xe)_trapped = 24.4 was used to resolve SW from trapped Xe. “n.d.” stands for light Xe isotopes in blanks which were too small to be determined.