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Fig. 6

image

Sequence of EIS maps showing the Fe xiv intensity (first row), Fe xvi intensity (second row), and Doppler shift (from 50 km s-1 to +50 km s-1, third row), Fe xxiii intensity (fourth row) and Fe xxiii blue wing intensity (fifth row, see text) for different rasters over time (from left to right) for the C4.7 class flare. The last column shows the closest AIA images in the 211, 335, and 131 Å filters, to the EIS Raster 3 (middle column). Footpoints K1 and K2 are indicated in the Fe xvi intensity and Doppler shift images in the Raster 3 (third column).

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