Fig. 6.
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1D histograms of the inferred magnetic field B [G] and thermal number density, nth [cm−3], during the entire analyzed flare duration. The strong narrow bin in the nth histogram at nth ≈ 2 × 1010 cm−3 is an artifact of a restricted EOVSA spectral range, as this number density is associated with the plasma frequency of 1.25 GHz (the smallest available frequency).
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