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Table 1
Lines used in the present work.
| Ion | Wvl. (Å) | log Tmax | G(Tmax) | Ion | Wvl. (Å) | log Tmax | G(Tmax) | ||
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| O iii | 702.900 | 4.90 | 1.13e-13 | S ix | 871.726 | 6.05 | 1.97e-16 | ||
| O iv | 787.710 | 5.17 | 1.00e-12 | S x | 264.231 | 6.18 | 7.31e-15 | ⋆ | |
| O v | 629.732 | 5.37 | 7.60e-12 | ⋆ | S xi | 281.402 | 6.28 | 2.45e-15 | ⋆ |
| O vi | 1031.914 | 5.48 | 2.91e-12 | ⋆ | S xii | 288.421 | 6.35 | 4.76e-15 | ⋆ |
| Ne iv | 543.887 | 5.21 | 6.53e-14 | S xiii | 256.685 | 6.42 | 1.75e-14 | ⋆ | |
| Ne v | 572.336 | 5.42 | 1.00e-13 | Fe viii | 185.213 | 5.62 | 9.55e-14 | ⋆ | |
| Ne vi | 558.685 | 5.59 | 1.02e-13 | Fe ix | 171.073 | 5.87 | 5.24e-13 | ⋆ | |
| Ne vii | 465.220 | 5.71 | 5.47e-13 | Fe x | 177.240 | 6.04 | 1.12e-13 | ⋆ | |
| Ne viii | 770.410 | 5.80 | 2.54e-13 | Fe xi | 182.169 | 6.13 | 2.87e-14 | ⋆ | |
| Mg v | 276.579 | 5.45 | 2.51e-14 | ⋆ | Fe xii | 193.509 | 6.19 | 9.84e-14 | ⋆ |
| Mg vi | 270.391 | 5.63 | 2.11e-14 | ⋆ | Fe xiii | 202.044 | 6.25 | 6.58e-14 | ⋆ |
| Mg vii | 276.154 | 5.78 | 9.33e-15 | ⋆ | Fe xiv | 264.790 | 6.29 | 5.79e-14 | ⋆ |
| Mg viii | 782.364 | 5.90 | 6.18e-15 | Fe xv | 284.163 | 6.34 | 3.18e-13 | ⋆ | |
| Mg ix | 706.036 | 5.99 | 1.95e-14 | Fe xvi | 262.976 | 6.43 | 1.10e-14 | ⋆ | |
| Mg x | 609.794 | 6.07 | 1.54e-13 | Fe xvii | 204.665 | 6.61 | 9.20e-16 | ⋆ | |
| Si vi | 246.003 | 5.61 | 2.91e-14 | ⋆ | Fe xviii | 974.860 | 6.86 | 7.91e-15 | |
| Si vii | 275.361 | 5.78 | 6.15e-14 | ⋆ | Fe xix | 1118.057 | 6.95 | 5.14e-15 | |
| Si viii | 276.850 | 5.93 | 1.13e-14 | Fe xx | 132.840 | 7.01 | 7.55e-15 | ||
| Si ix | 258.082 | 6.05 | 3.18e-15 | ⋆ | Fe xxi | 1354.067 | 7.06 | 1.27e-14 | |
| Si x | 258.371 | 6.15 | 3.78e-14 | ⋆ | Fe xxii | 845.571 | 7.11 | 6.10e-15 | |
| Si xi | 580.920 | 6.22 | 9.08e-15 | Fe xxiii | 263.766 | 7.17 | 1.73e-15 | ||
| Si xii | 520.666 | 6.30 | 4.48e-14 | Fe xxiv | 192.029 | 7.26 | 1.17e-14 | ⋆ | |
| S viii | 198.554 | 5.91 | 3.93e-15 | ||||||
Notes. Tmax: temperature of maximum ion abundance. G(Tmax): line emissivity at Tmax. Stars indicate the ions whose lines can be observed by the Hinode/EIS spectrometer (although EIS lines may be different from those listed here).
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