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Fig. 9


Same as for Fig. 8 for the predicted spectra in 2004 (dashed curves), assuming that i) the lower part of the corona, with thickness h3 is isothermal at 620 kK with thickness h3; ii) the temperature in the upper part is 1.5 MK; and iii) Te = TH elsewhere. Curves are labeled with the thickness h3 (Mm).

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