\begin{table}%t1 \caption{\label{tab:irradiances}Irradiances in $\mu$W m$^{-2}$.} %\centerline {\small \begin{tabular}{@{}llrrrrl@{}} \hline\hline \noalign{\smallskip} Spectral lines & $\lambda$ (nm) & PEVE & $P$ & {\it SN} & $S$ & \\ \hline\noalign{\smallskip} \ion{He}{ii} (bl \ion{Si}{xi}) & 30.400 & 309 & 663 & 502 & 395 & \\ \ion{Si}{viii} & 31.983 & 8.2 & 11.7 & 12.5 & 7.6 & \\ \ion{Fe}{xvi} (bl \ion{Mg}{viii}) & 33.530 & 2.7 & 2.0 & 1.8 & 1.2 & \\ \ion{Mg}{viii} (bl) & 33.901 & 1.9 & 1.8 & 1.8 & 1.1 & \\ \ion{Si}{x} (bl) & 34.750 & 5.6 & 6.3 & 6.8 & 4.3 & \\ \ion{Si}{ix} (bl) & 34.987 & 5.1 & 5.6 & 5.9 & 3.7 & \\ \ion{Si}{x} (bl) & 35.601 & 3.3 & 4.0 & 3.7 & 2.3 & \\ \ion{Mg}{ix} (bl \ion{Mg}{vii}) & 36.800 & 42. & 39.4 & 41.5 & 28.3 & \\ & & & & & \\ \ion{He}{i} & 51.562 & 1.2 & 1.0 & 1.3 & 0.87 & \\ \ion{Si}{xii} & 52.066 & 0.67 & 0.82 & 0.93 & 0.70 & \\ \ion{He}{i} (bl) & 52.221 & 1.9 & 1.5 & 1.7 & 1.3 & \\ \ion{O}{iii} & 52.600 & 2.6 & 2.2 & 2.3 & 1.9 & \\ \ion{He}{i} (bl) & 53.703 & 5.2 & 4.9 & 4.6 & 4.0 & \\ \ion{Ne}{iv} & 54.207 & 0.66 & 0.51 & 0.46 & 0.34 & \\ \ion{Ne}{iv} (sbl) & 54.400 & 1.1 & 0.84 & 0.74 & 0.52 & \\ \ion{O}{iv} (sbl) & 55.450 & 26.4 & 25.4 & 21.6 & 20.8 & \\ \ion{Ne}{vi} (2) (bl) & 56.280 & 2.3 & 2.1 & 1.9 & 1.5 & \\ \ion{Ne}{v} (2) & 56.982 & 0.80 & 0.62 & 0.61 & 0.44 & \\ \ion{Ne}{v} (3) & 57.233 & 1.2 & 1.1 & 1.1 & 0.81 & \\ \ion{C}{iii} (bl \ion{Ca}{x}) & 57.420 & 1.1 & 1.0 & 1.0 & 0.75 & \\ \ion{He}{i} & 58.400 & 48. & 36. & 33. & 78. & \\ \ion{Ar}{vii} & 58.575 & 0.89 & 0.60 & 0.55 & 1.3 & \\ \ion{O}{iii} & 60.000 & 5.2 & 4.8 & 4.0 & 3.0 & \\ \ion{Mg}{x} (bl \ion{O}{iv}) & 61.000 & 16. & 14.3 & 11.5 & 9.6 & \\ \ion{Mg}{x} (bl) & 62.500 & 6.6 & 5.8 & 5.1 & 3.9 & \\ \ion{O}{v} & 63.000 & 56. & 35. & 33. & 35. & \\ \hline \end{tabular}} \tablefoot{PEVE are the irradiances from the prototype-EVE, Apr 14, 2008. P are the irradiances from the full-Sun NIS observation of Mar 17, 2008, obtained with the Del Zanna (2001) scaled responsivities and the present long-term corrections; SN are the NIS irradiances of the same observation obtained with the current standard CDS responsivities (version~4, 2002) and the present long-term corrections; S are the same NIS irradiances obtained with the current standard CDS responsivities (version~4, 2002) and the standard long-term corrections.} \end{table}