Fig. 9.

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SoloHI height vs. time map for 30 and 31 March. The map is generated by taking a strip of images at a given position angle, in this case, 86° from solar north, and stacking each time step together. The extended horizontal black line is the boundary between detectors. The y-axis is the radial distance in R. The features highlighted in Fig. 8 are also noted here, as are various pointing changes caused by the spacecraft. Notably, the location of the tracks seem unaffected by these changes.

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