Fig. 2.
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SOL2017-04-23 flare. The ALMA images are difference images between the designated time frame and the base preflare frame. The other are regular full-scale images. ALMA contours outline five levels equidistantly within the range of 100−500 K. The peak ALMA brightness in the flaring region is marked with a white “x”. The intensity was clipped in each image to better show structures of interest.
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