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Fig. 13.


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Height-time diagram for the CME on August 14, 2010, combining measurements made using observations by different EUV imagers and coronagraphs. The measurement errors were obtained by remeasuring the position of the flux rope several times in sample images. We then applied error propagation to the standard deviation of these measurements to obtain the error bars shown here. The COR1 datapoints (in yellow) show the largest error bars because it was more difficult to define the exact position of the flux rope in those images.

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