Table 2: Comparison between our solar abundances (second Col.) and those of Grevesse & Sauval (2000) (third column). For iron, the abundance value obtained using ionised lines is also given. The number of lines and the standard deviation of the measurements for each species are also reported in the fourth and in the fifth column respectively. When only three or two lines are measured (sodium and aluminum), half of the difference between the maximum and minimum value is reported instead of the standard deviation.

X	A(X)		Number
			of lines
Fe I	7.52	7.50	66	0.03
Fe II	7.57	7.50	11	0.03
Na I	6.37	6.33	3	0.11
Al I	6.47	6.47	2	0.02
Si I	7.56	7.55	9	0.03
Ca I	6.36	6.36	11	0.03
Ti I	4.97	5.02	11	0.02
Cr I	5.65	5.64	6	0.06
Ni I	6.25	6.25	23	0.04

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