Fig. 2.


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Large (>100 nT) SFEs on (a) 28 October 2003, and (b) 4 November 2003. In each case, the associated SXR burst (top panel) is shown along with the magnetometer traces (bottom three panels). The vertical dashed lines are drawn at the peak of the SXR event. (From Cliver & Svalgaard 2004, with permission of Solar Physics.)

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