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Fig. 6.

image

Kinematics of the moving radio bursts and Type II lanes in relation to the CME expansion. The Type II bursts and CME kinematics were previously studied by Palmerio et al. (2019). The figure is adapted from Palmerio et al. (2019), to which we included the three moving radio sources studied here. The EUV measurements are taken with PROBA2/SWAP and STEREO/EUVI-A, the white-light ones with LASCO/C2–C3 and STEREO/COR1–COR2-A, and the radio ones with NDA and the WAVES instruments onboard Wind (Ogilvie & Desch 1997) and both STEREO spacecraft.

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