Fig. 8.

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Roughly cotemporal images of the 30 March CME from SoloHI and the SECCHI instrument suite. To highlight the common FoV, images from all SoloHI tiles and COR2 and HI1 are projected onto identical grids, covering 6–50 R⊙ in the radial direction and −22 to 22 R⊙ in the y-direction. The SoloHI images are flipped from their standard viewing direction to facilitate comparison. Features of note are highlighted in the earliest frame in which they are all visible in both instruments to facilitate tracking these features in the frames. All images from every instrument were processed with a running ratio byte-scaled to a range of 0.98–1.02. The times given in the SoloHI frames correspond to the time of the tile 1 image, and the other tiles are the closest frame to that tile 1 image. Similarly, SECCHI times are based on COR2 timing, and the closest HI1 frame was selected. Movies of the projected FoVs used to generate these panels are provided online for both SECCHI and SoloHI covering the entire period of 28 March to 2 April.
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