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.
$\Delta h$ /km Fig. 6a Fig. 8a (N) Fig. 8b (S-W)

peak average peak average

Hump 2 90 0 80 0 40

Hump 3 -50 0 -210 0 -60

Continuum 540 540 470 270 320

N I 270 0 120 180 130

S I -180 0 160 0 100

C III 3300

**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.
$\Delta h$ /km	Fig. 6a	Fig. 8a (N)	Fig. 8b (S-W)
		peak	average	peak	average
Hump 2	90	0	80	0	40
Hump 3	-50	0	-210	0	-60
Continuum	540	540	470	270	320
N I	270	0	120	180	130
S I	-180	0	160	0	100
C III	3300

Source LaTeX | All tables | In the text

	1 Introduction
	2 The SUMER instrument
	3 Observations and data analysis
	4 Interpretation
	5 Conclusion
	References