Fig. 1.

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Orbital configuration in HEE coordinates of the analysed spacecraft during the event. Black arrow shows the longitude of the AR at the moment of the eruption. Earth’s magnetospheric bow shock (orange) and magnetopause (purple) are calculated as in Ipavich et al. (1981) with a speed of 500 km s−1 (black line indicates the bow shock without the influence of the SW). Crosses in Earth’s perspective indicate the Lagrange points. Earth’s radius is scaled by a factor of 4. Sun not to scale. The x, y, and z scales are different in some of the panels.
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