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Table 1
EIS spectral lines used in paper.
| Ion | Wavelength (Å) | log T |
|
|
||
| Cool lines | ||
| Si vii | 275.36 | 5.80 |
| Fe viii (bl,c) | 186.60 | 5.80 |
| Coronal and Hot lines | ||
| Fe xi | 188.23 | 6.15 |
| Fe xii | 192.39 | 6.20 |
| Fe xv | 284.16 | 6.35 |
| S xiii (bl,c) | 256.68 | 6.40 |
| Fe xvi | 262.97 | 6.45 |
| Ca xiv | 193.87 | 6.55 |
| Ca xv (bl,c) | 200.97 | 6.65 |
| Ca xvii (bl,c) | 192.85 | 6.75 |
| Flare lines | ||
| Fe xxiii | 263.76 | 7.15 |
| Fe xxiv (bl) | 192.02 | 7.25 |
Notes. Blended lines are marked with (bl) and corrected blends are marked with (c). log T is the logarithm of the formation temperature of the ion. They correspond to the peaks of the curves in Fig. 4.
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