Table 4: Solar elemental abundances. Column 1 indicate the elements and ions and Cols. 2 and 3 give the meteoritic and solar photospheric standard abundances from Grevesse & Sauval (1998). Our solar abundances are given in Cols. 4 and 5 gives the differences between this study and the photospheric values. Asterisks indicate that we have used astrophysical $\log gf$ -values and thereby forced the abundance to the standard photospheric value. Asterisks in parenthesis indicate that some of the lines have astrophysical $\log gf$ -values.
Ion Meteorites Photosphere This study Diff.

Fe I 7.50 7.50 7.56 +0.06

Fe II 7.50 7.50 7.58 +0.08

Na I 6.32 6.33 6.27 -0.06

Mg I 7.58 7.58 7.58 *

Al I 6.49 6.47 6.47 *

Si I 7.56 7.55 7.54 -0.01(*)

Ca I 6.35 6.36 6.36 *

Ti I 4.94 5.02 4.92 -0.10

Ti II 4.94 5.02 4.91 -0.11

Cr I 5.69 5.67 5.67 *

Cr II 5.69 5.67 5.67 *

Ni I 6.25 6.25 6.24 -0.01(*)

Zn I 4.67 4.60 4.60 *

**Table 4:** Solar elemental abundances. Column 1 indicate the elements and ions and Cols. 2 and 3 give the meteoritic and solar photospheric standard abundances from Grevesse & Sauval (1998). Our solar abundances are given in Cols. 4 and 5 gives the differences between this study and the photospheric values. Asterisks indicate that we have used astrophysical $\log gf$ -values and thereby forced the abundance to the standard photospheric value. Asterisks in parenthesis indicate that some of the lines have astrophysical $\log gf$ -values.
Ion	Meteorites	Photosphere	This study	Diff.
Fe I	7.50	7.50	7.56	+0.06
Fe II	7.50	7.50	7.58	+0.08
Na I	6.32	6.33	6.27	-0.06
Mg I	7.58	7.58	7.58	*
Al I	6.49	6.47	6.47	*
Si I	7.56	7.55	7.54	-0.01(*)
Ca I	6.35	6.36	6.36	*
Ti I	4.94	5.02	4.92	-0.10
Ti II	4.94	5.02	4.91	-0.11
Cr I	5.69	5.67	5.67	*
Cr II	5.69	5.67	5.67	*
Ni I	6.25	6.25	6.24	-0.01(*)
Zn I	4.67	4.60	4.60	*

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