All Tables

Table 1: Linear correlation coefficients, r, between the chromospheric network maps shown in Fig. 3. Upper part: with respect to hump 1; lower part: with respect to C III lines. Values for the total areas are given as well as for the lane and cell regions.
Table 2: Height differences, $\Delta h$ , of solar emission with respect to the hump 1 obtained by cross-correlations calculations between limb brightening curves from slit (Fig. 6a) and hole (Fig. 8) observations. The rows named "average'' refer to averages above the horizontal dashed-dotted lines.