Fig. 3.
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Panel a: STEP magnet channel ion flux summed over all energy channels and panel b: HET C detector high-gain channel count rates overplotted on the trajectory of Solar Orbiter in cylindrical VSO coordinates. Empirically derived estimates of the bow shock location (Shan et al. 2015), as well as upper mantle and lower mantle boundaries (Martinecz et al. 2009) are overplotted for reference.
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