Table 2: The calculated abundances relative to Fe, obtained from the EMD analysis of the Chandra (quiescence) and XMM-Newton (flare). "Flare'' abundances are in fact averaged "quiescence+flare'' components during the 2001 flare observed by XMM-Newton. Uncertainties are 1 $\sigma$ .
Flare Quiescence Ratio

Element X/Fe X/Fe Flare/Quies.

N
15.1 $\pm$ 2.7 13.7 $\pm$ 2.3 1.1 $\pm$ 0.3

O 30.3 $\pm$ 5 42 $\pm$ 6 0.72 $\pm$ 0.15

Ne 15.2 $\pm$ 2.3 19.9 $\pm$ 2 0.76 $\pm$ 0.14

Mg 1.94 $\pm$ 0.33 1.66 $\pm$ 0.17 1.17 $\pm$ 0.23

Si 0.99 $\pm$ 0.4 1.37 $\pm$ 0.14 0.72 $\pm$ 0.30

**Table 2:** The calculated abundances relative to Fe, obtained from the EMD analysis of the *Chandra* (quiescence) and *XMM-Newton* (flare). "Flare'' abundances are in fact averaged "quiescence+flare'' components during the 2001 flare observed by *XMM-Newton*. Uncertainties are 1 $\sigma$ .
	Flare	Quiescence	Ratio
Element	X/Fe	X/Fe	Flare/Quies.
N	15.1 $\pm$ 2.7	13.7 $\pm$ 2.3	1.1 $\pm$ 0.3
O	30.3 $\pm$ 5	42 $\pm$ 6	0.72 $\pm$ 0.15
Ne	15.2 $\pm$ 2.3	19.9 $\pm$ 2	0.76 $\pm$ 0.14
Mg	1.94 $\pm$ 0.33	1.66 $\pm$ 0.17	1.17 $\pm$ 0.23
Si	0.99 $\pm$ 0.4	1.37 $\pm$ 0.14	0.72 $\pm$ 0.30

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