Table 1: Observed offset of the network contrast for 19 emission lines. Lines from the same raster are co-temporal, raster start and stop time are in UTC.

Line
$\lambda $ / Å log T/K $\Delta \lambda$ / Å Time
Mg  IX 749.54 6.0 0.017 01:44-02:35
IV 750.22 5.0 0.124 01:44-02:35
IV 765.15 5.1 0.172 02:37-03:28
Ne  VIII 780.30 5.8 0.002 02:37-03:28
V 786.47 5.26 0.143 02:37-03:28
IV 787.72 5.23 0.174 02:37-03:28
V 761.99 5.4 0.136 02:37-03:28
II 833.32 4.5 0.075 03:30-04:20
III 833.74 4.9 0.155 03:30-04:20
III 977.03 4.8 0.142 05:15-06:06
II 1037.00 4.4 0.109 06:08-06:59
VI 1031.93 5.5 0.134 06:08-06:59
II 1083.99 4.4 0.053 07:01-07:52
Si  III 1206.51 4.7 0.161 07:54-08:45
V 1238.82 5.3 0.157 08:48-09:39
Si  II 1309.28 4.26 0.024 10:33-11:24
Ni  II 1317.22 4.1 -0.007 10:33-11:24
I 1318.98 4.0 -0.009 10:33-11:24
Si  IV 1402.77 4.9 0.151 11:26-12:17


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