Table 1: List of lines synthesised in this work, and with the logarithm of the temperature of their maximum emission. These lines can be observed by SOHO/SUMER (Ne VIII, Mg X, Fe XVIII, Fe XIX), SOHO/EIT (Fe IX, Fe XII) and Hinode/EIS (Fe IX, Fe XII, Fe XXIV).
$\log~(T_{\rm max})$ Li-like Others

5.8 Ne VIII 770.41 Å Fe IX 171.07 Å

6.1 Mg X 624.94 Å Fe XII 195.12 Å

6.8 Fe XVIII 974.86 Å

6.9 Fe XIX 1118.06 Å

7.24 Fe XXIV 192.03 Å

**Table 1:** List of lines synthesised in this work, and with the logarithm of the temperature of their maximum emission. These lines can be observed by SOHO/SUMER (Ne VIII, Mg X, Fe XVIII, Fe XIX), SOHO/EIT (Fe IX, **Fe XII**) and Hinode/EIS (Fe IX, Fe XII, Fe XXIV).
$\log~(T_{\rm max})$	Li-like	Others
5.8	Ne VIII 770.41 Å	Fe IX 171.07 Å
6.1	Mg X 624.94 Å	Fe XII 195.12 Å
6.8		Fe XVIII 974.86 Å
6.9		Fe XIX 1118.06 Å
7.24	Fe XXIV 192.03 Å

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