Determination of the acceleration region size in a loop-structured solar flare

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Fig. 5

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Flare loop lengths for each 2-keV electron energy bin, for the same five time intervals as in Fig. 4. a) Results from forward-fit algorithm; b) Results from uv-smooth method. The solid curves represent the fits of the model described in Eq. (11). The χ² of the fittings are also shown.

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