Foreshock compressive structures start at similar normalized distances in both IP and planetary shocks when suprathermal ions reach ~1% density, but IP shocks show no mature high-amplitude SLAMS because of limited growth zones and absent global curvature.
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Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.
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Compressive Structures in the Foreshock of Collisionless Shocks
Foreshock compressive structures start at similar normalized distances in both IP and planetary shocks when suprathermal ions reach ~1% density, but IP shocks show no mature high-amplitude SLAMS because of limited growth zones and absent global curvature.