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Table A.1.
Selected emission lines observed by SDO/EVE and AIA with corresponding wavelength λ, primary ion species, and formation temperature T (both logarithmic and absolute).
| EVE Lines | |||
|---|---|---|---|
| λ (nm) | Ion(s) | logT | T (K) |
| 13.29 | Fe XX | 7.0 | 107 |
| 33.54 | Fe XVI | 6.4 | 2.5 × 106 |
| 17.11 | Fe IX | 5.8 | 6.3 × 105 |
| 30.38 | He II | 4.8 | 6.3 × 104 |
| AIA Filters | |||
| λ (nm) | Ion(s) | logT | T (K) |
| 13.1 | Fe VIII, Fe XXI | 5.6, 7.0 | 4 × 105, 107 |
| 33.5 | Fe XVI | 6.4 | 2.5 × 106 |
| 17.1 | Fe IX | 5.8 | 6.3 × 105 |
| 30.4 | He II | 4.7 | 5 × 104 |
| 160.0 | Continuum | 3.7 | 5 × 103 |
Notes. Adapted from Woods et al. (2012) and Lemen et al. (2012).
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