\begin{table}%t3 \caption{\label{comp.clementini}Comparison between the atmospheric ion abundances relative to the Sun obtained by Clementini et~al. (\cite{Clementini1995}) and in this work. } \small%\centering \par \begin{tabular}{lccc} \hline \hline\noalign{\smallskip} Ion &\multicolumn{3}{c}{[$N_{\rm el}/N_{\rm H}$]$_{\rm Sun}$} \\ & \multicolumn{2}{c}{This work} & Clementini et~al. (\cite{Clementini1995}) \\ \hline \ion{O}{i} & ~$-$0.60~$\pm$~0.04 & ~$-$0.59~$\pm$~0.04 & ~$-$0.69 \\ \ion{Na}{i} & ~$-$1.51~$\pm$~0.05 & ~$-$1.51~$\pm$~0.05 & ~$-$1.39 \\ \ion{Mg}{i}~ & ~$-$1.03~$\pm$~0.10 & ~$-$0.97~$\pm$~0.14 & ~$-$1.08~$\pm$~0.07 \\ \ion{Al}{i} & ~$-$0.92~$\pm$~0.26 & ~$-$0.90~$\pm$~0.26 & ~$-$1.89 \\ \ion{Si}{i} & ~$-$1.03~$\pm$~0.11 & ~$-$1.02~$\pm$~0.11 & ~$-$0.92~$\pm$~0.02 \\ \ion{Si}{ii} & ~$-$1.08~$\pm$~0.04 & ~$-$1.01~$\pm$~0.08 & ~$-$1.14 \\ \ion{Ca}{i} & ~$-$1.25~$\pm$~0.05 & ~$-$1.17~$\pm$~0.09 & ~$-$1.07~$\pm$~0.05 \\ \ion{Sc}{ii} & ~$-$1.18~$\pm$~0.13 & ~$-$1.19~$\pm$~0.09 & ~$-$1.35~$\pm$~0.12 \\ \ion{Ti}{i} & ~$-$1.19~$\pm$~0.08 & ~$-$1.18~$\pm$~0.07 & ~$-$1.20~$\pm$~0.06 \\ \ion{Ti}{ii} & ~$-$1.07~$\pm$~0.19 & ~$-$1.08~$\pm$~0.13 & ~$-$1.05~$\pm$~0.18 \\ \ion{Cr}{i} & ~$-$1.58~$\pm$~0.09 & ~$-$1.54~$\pm$~0.09 & ~$-$1.41~$\pm$~0.18 \\ \ion{Cr}{ii} & ~$-$1.30~$\pm$~0.11 & ~$-$1.26~$\pm$~0.10 & ~$-$1.33~$\pm$~0.14 \\ \ion{Mn}{i} & ~$-$1.82~$\pm$~0.15 & ~$-$1.77~$\pm$~0.12 & ~$-$1.99~$\pm$~0.12 \\ \ion{Fe}{i} & ~$-$1.48~$\pm$~0.12 & ~$-$1.44~$\pm$~0.11 & ~$-$1.39~$\pm$~0.13 \\ \ion{Fe}{ii} & ~$-$1.34~$\pm$~0.13 & ~$-$1.30~$\pm$~0.10 & ~$-$1.39~$\pm$~0.13 \\ \ion{Ni}{i} & ~$-$1.54~$\pm$~0.08 & ~$-$1.52~$\pm$~0.08 & ~$-$1.47 \\ \ion{Zn}{i} & ~$-$1.57~$\pm$~0.01 & ~$-$1.55~$\pm$~0.01 & ~$-$1.35 \\ \ion{Y}{ii} & ~$-$1.48~$\pm$~0.09 & ~$-$1.47~$\pm$~0.09 & ~$-$1.50 \\ \ion{Ba}{ii} & ~$-$1.36~$\pm$~0.22 & ~$-$1.48~$\pm$~0.08 & ~$-$1.39~$\pm$~0.12 \\ \noalign{\smallskip} \vmic & 3.1~\kms & Depth dep. & ~4.2~\kms \\ \hline \end{tabular} \end{table}