All Tables

• Table 1: The first two columns are explicit. The third column shows the number of SUMER data files used to compute the average intensity. The fourth column shows (in percent) the statistical standard deviation of the averaged intensity, while the fifth column shows the averaged intensity. The sixth column shows intensity values from NRLEUV. The seventh column gives, when available, values from: ¹ Wilhelm et al. (1998), observed near disk center. ² Wilhelm et al. (1998), mean intensity deduced from full Sun observation. All intensities are in mW m^-2 sr^-1.
• Table 2: Calculated and observed mean intensities for optically thin lines used in the DEM computation. The first three columns are explicit. The fourth column shows the number of SUMER data files used to compute the mean intensity. The fifth column shows (in percent) the statistical standard deviation of the mean intensity. The sixth and seventh columns show the mean (or "observed'') and calculated intensity. The eighth column shows their ratio.
• Table 3: Numerical values for the quiet sun DEM. DEM is in cm^-5 K^-1.
• Table 4: Intensity (in mW m^-2 sr^-1) for strong optically thin lines.