The Sun as an X-ray star - V. A new method to retrieve coronal filling factors

Open Access

Fig. 2.

EMDs of C5.8, M1.0, M1.1, M2.8, M4.2, M7.6, and X1.5 flares as presented by Reale et al. (2001) (individual colors) along with their weighted average EMD (FL-AVG, blue). The y-axis shows the emission measure per unit area, in units of 10⁴⁴ cm⁻⁵.

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