Table 1
Emission lines and AIA/SDO bands synthesized from 3D MHD model.
| Line | Wavelength | Formation temperature |
| [Å] |
|
|
|
|
||
| O vi | 1032 | 5.5 |
| Mg x | 625 | 6.0 |
| AIA / He i | 304 | 4.9 |
| AIA / Fe ix/x | 171 | 5.9 |
Notes. For O vi and Mg x, the line formation temperature is given, i.e., the temperature where G(T) ∝ (nion/nel) T−1/2 exp[− hν/(kBT)] reaches its maximum value (assuming ionization equilibrium). For the AIA bands, the main contributing lines are given along with the center wavelength and the formation temperature of the plasma dominating the emission in the respective band.
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