Fig. 2.

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Location of Solar Orbiter in HEE coordinates at the onset of the various events alongside the approximate SoloHI FoV at each time. For each event, the spacecraft is consistently near 0.32 au, meaning that the SoloHI FoV is roughly 6 − 50 R⊙, as shown with the dashed lines coming from the spacecraft. The arrows indicate the longitude of the active region at the time of the associated flare, also shown in Table 2. These do not necessarily coincide with the direction of propagation of the CME. The dashed circles represent intervals of 0.25 au from the Sun. The solid black ellipse is the orbit of Solar Orbiter. The Earth and STEREO-A are also shown for reference. The position of the Earth can be taken for that of LASCO. The solid circles representing the various objects are not to scale.
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