Magnetic connectivity of coronal loops and flare-accelerated electrons in a B-class flare - Based on X-ray, EUV (DEM analysis), and type-III radio burst observations

Open Access

Fig. 10.

Type-III radio source positions for burst R5₀⁶ to R7_g² (flare phases are noted in the sub-captions). The colors of the contours correspond to their frequency, namely 80 MHz (purple), 70 MHz (blue), 60 MHz (green), 50 MHz (orange) and 40 MHz (red). The gray lines are the lines of longitude and latitude of the AR.

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