Formation and dynamics of transequatorial loops | Astronomy & Astrophysics (A&A)

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Fig. 12.

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Emission measure (EM) loci curves for the bright point, corresponding to “P2” (in Figs. 5 and 9), derived with spectral line observations during E2. The histograms representing number of crossings within a given temperature bin are plotted. No background/foreground emission has been accounted for.

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