Table 2.
Analysed spectral lines with EIS, IRIS and SPICE.
| Instrument | Spectral line | λ [Å] | log(T [K]) |
|---|---|---|---|
| IRIS | Mg II | 2795.5 | 4.5 |
| H Lyman β | 1025.72 | 4.0 | |
| C III | 977.03 | 4.5 | |
| SPICE | N IV | 765.15 | 5.1 |
| (Solar Orbiter ) | O VI | 1031.93 | 5.5 |
| Ne VIII | 770.42 | 5.8 | |
| Mg IX | 706.02 | 6.0 | |
| Fe XVIII | 974.84 | 6.9 | |
| EIS (Hinode) | He II | 256.32 | 4.9 |
| Fe VIII | 194.66 | 5.7 | |
| Fe XII | 195.12 | 6.2 | |
| Fe XV | 284.16 | 6.4 | |
| Fe XXIV | 192.03 | 7.3 | |
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