Table 2.
Intensities averaged over the X-region (“P”), TELs (“L”’), hot loops beneath the X-region (“D”), the bright region hosting recurrent brightenings (“P2”) and region considered for background/ foreground assessment (“B”), respectively in Fig. 9.
| Fe lines | E1 | E2 | E3 | E4 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| P | L | D | P2 | B | P | L | D | P2 | B | P | L | D | P2 | B | P | L | D | P2 | B | |
| Fe VIII | 568.0 | 420.4 | 411.3 | – | 568.0 | 274.0 | 597.3 | 498.4 | 136.6 | 128.4 | 165.8 | 482.2 | 411.8 | – | 1335.3 | 488.0 | 421.8 | 799.9 | – | 5273.9 |
| Fe IX | 69.2 | 190.2 | 124.3 | – | 46.3 | 174.7 | 205.4 | 129.5 | 21.1 | 362.6 | 117.6 | 156.0 | 130.8 | – | 85.3 | 201.2 | 185.8 | 285.1 | – | 17.0 |
| Fe X | 516.9 | 1203.6 | 1003.2 | – | 228.1 | 1171.1 | 957.3 | 977.0 | 512.4 | 289.4 | 802.7 | 937.8 | 964.2 | – | 1990.9 | 962.6 | 928.8 | 1711.2 | – | 1312.1 |
| Fe XI | 2096.8 | 4222.3 | 4499.5 | – | 2114.4 | 4382.8 | 3267.3 | 4234.2 | 1551.1 | 6534.7 | 3586.7 | 3505.8 | 4249.4 | – | 13723.4 | 3761.4 | 3566.7 | 5950.9 | – | 26928.2 |
| Fe XII | 794.5 | 1394.2 | 1597.9 | – | 178.2 | 1132.8 | 952.8 | 1406.4 | 610.7 | 167.0 | 1203.0 | 986.9 | 1629.8 | – | 166.1 | 1110.1 | 1217.3 | 1951.2 | – | 170.2 |
| 192 Å | ||||||||||||||||||||
| Fe XII | 2804.1 | 4832.1 | 5484.3 | – | 638.8 | 4095.9 | 3504.4 | 4976.8 | 2141.3 | 592.2 | 4165.0 | 3547.3 | 5607.1 | – | 593.9 | 3934.5 | 4297.9 | 6630.3 | – | 619.4 |
| 195 Å | ||||||||||||||||||||
| Fe XIII | 1688.0 | 2412.1 | 3123.3 | – | 269.8 | 1211.6 | 1702.9 | 2535.9 | 1098.5 | 210.4 | 1946.6 | 1774.3 | 3345.8 | – | 215.0 | 1628.9 | 2129.9 | 3467.5 | – | 218.1 |
| Fe XIV | 695.3 | 738.8 | 1018.3 | – | 159.8 | 402.8 | 660.8 | 942.3 | 512.1 | 69.7 | 573.5 | 684.6 | 1114.8 | – | 193.3 | 538.0 | 737.3 | 981.0 | – | 53.9 |
| Fe XV | 4840.5 | 3927.6 | 6162.3 | – | 1183.1 | 1403.2 | 4113.0 | 6550.6 | 3175.2 | 451.3 | 2280.3 | 4854.3 | 6757.8 | – | 480.2 | 2667.8 | 4345.2 | 4909.9 | – | 448.8 |
Notes. The averaged intensities for Mg VII and Si VII are not noted here because the background averaged intensities exceed those in the region(s) under consideration for all four EIS observations.
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