Open Access
Table 2.
Line list used in this work from Parenti et al. (2005a) and GUN04.
| Ion | λth (Å) | log T (K) | QS | PRM1 | PRM04 | ||
|---|---|---|---|---|---|---|---|
| Si II | 1190.416 | 4.13 | 14.16 | 2.60 | 2.05 | ° | |
| Si II | 1197.3955 | 4.13 | 8.59 | 1.21 | ° | ||
| Si II | 1264.738 | 4.13 | 13.73 | ° | |||
| S II | 1253.811 | 4.25 | 11.89 | 1.20 | 0.67 | ° | |
| S II | 1250.585 | 4.25 | 5.04 | 0.37 | |||
| C II | 1036.337 | • | 4.37 | 33.01 | 10.94 | 6.40 | |
| C II | 1037.018 | • | 4.37 | 40.01 | 12.92 | 8.73 | |
| N II | 1085.701 | 4.38 | 43.55 | 11.48 | 6.20 | ||
| N II | 1083.990 | 4.38 | 10.84 | 2.64 | 1.32 | ||
| S III | 1015.496 | • | 4.46 | 0.88 | 0.18 | ||
| S III | 1200.959 | 4.46 | 7.98 | 1.53 | ° | ||
| S III | 1194.047 | 4.46 | 0.87 | ° | |||
| Si III | 1109.943 | 4.67 | 0.87 | ° | |||
| Si III | 1113.25 | 4.67 | 13.29 | 2.05 | ° | ||
| Si III | 1206.502 | 4.67 | 549.05 | 60.89 | |||
| C III | 977.020 | • | 4.85 | 518.55 | 211.91 | 277.8 | |
| C III | 1174.933 | 4.85 | 42.76 | ||||
| C III | 1175.7111 | 4.85 | 157.10 | 16.80 | 20.51 | ||
| Si IV | 1128.34 | 4.87 | 12.23 | 1.66 | 1.79 | ° | |
| Si IV | 1393.76 | 4.87 | 62.53 | ° | |||
| N III | 989.799 | • | 4.88 | 11.45 | 2.85 | 3.95 | |
| N III | 991.577 | • | 4.88 | 22.75 | 4.89 | 7.90 | |
| O III | 525.794 | • | 4.93 | 8.90 | 5.50 | ||
| O III | 703.850 | • | 4.93 | 20.0 | |||
| S IV | 1062.664 | 4.99 | 3.74 | 9.48 | 0.91 | ° | |
| S IV | 1072.974 | 4.99 | 7.56 | 1.58 | ° | ||
| C IV | 1548.187 | 5.03 | 103.55 | ||||
| N IV | 955.334 | • | 5.17 | 0.17 | 0.05 | ||
| O IV | 555.264 | 5.18 | 24.75 | ||||
| O IV | 1399.776 | 5.18 | 1.32 | ||||
| O IV | 1401.163 | 5.18 | 8.21 | ||||
| N V | 1238.821 | 5.27 | 57.24 | ||||
| N V | 1242.804 | 5.27 | 28.97 | ||||
| O V | 1218.347 | 5.37 | 62.76 | 16.08 | 17.59 | ||
| Ne V | 572.113 | 5.46 | 2.45 | 0.63 | |||
| Ne V | 1145.582 | 5.46 | 1.04 | ||||
| O VI | 1031.912 | • | 5.48 | 247.78 | |||
| O VI | 1037.614 | • | 5.48 | 116.13 |
Notes. The intensities are given in erg cm−2 s−1 sr−1. The lines indicated with “°” extend the lists published in Parenti et al. (2005a) and GUN04. The lines marked with “•” will be measured by Solar Orbiter/SPICE.
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