Table 3
List of the EIS observed emission lines used to constrain DEM curves.
| EIS observed lines | λ | log Tmax | Observed | Predicted | Observed | Predicted | |
| used for the DEM | (Å) | (K) | (spire) | (spire) | (footpoint) | (footpoint) | |
|
|
|||||||
| Fe VIII (bl) | 186.605 | 5.8 | 445 | 562 (26%) | 1617 | 1982 (23%) | |
| Fe XII | 195.119 | 6.2 | 1707 | 1755 (3%) | 3270 | 3415 (4%) | |
| Si X | 261.056 | 6.2 | 408 | 298 (–27%) | 790 | 629 (–20%) | |
| Mg VI | 268.991 | 5.7 | 106 | 62 (–42%) | 355 | 240 (–32%) | |
| Fe XV (bl) | 284.160 | 6.4 | 9221 | 9943 (8%) | 16270 | 17170 (6%) | |
Notes. Column 4 and 5 represents observed and predicted intensities (obtained from the EIS DEM) for the jet-spire region; Cols. 6 and 7 represents observed and predicted intensities (obtained from the EIS DEM) for the jet-footpoint region; EIS intensities are in erg cm-2 s-1 sr-1 units, bl – blended lines; and percentage difference between observed and predicted intensities are given in parenthesis in Cols. 5 and 7.
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