Fig. 6.


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Data from SDO on 28 May 2020 at 16:45 UT, of the same region as the SPICE raster shown in Fig. 3. Here we show (a) the photospheric line-of-sight magnetogram from HMI, saturated at ±50 G, (b) the 30.4 nm channel from AIA corresponding to the transition region emission as seen by SPICE in C III, and (c) the 17.1 nm channel from AIA corresponding to the coronal emission as seen by SPICE in Ne VIII. The yellow circle highlights the brightening also highlighted in Fig. 3. The SDO maps are projected onto the area as seen by SPICE and interpolated to a pixel scale of 435 km on the Sun that corresponds to AIA image scale of 0.6″ per pixel.

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