Solar Orbiter data reveals SEP flux deflections associated with magnetic flux tubes, positioning SEPs as a diagnostic for solar wind structures.
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Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification 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.
citing papers explorer
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Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter
Solar Orbiter data reveals SEP flux deflections associated with magnetic flux tubes, positioning SEPs as a diagnostic for solar wind structures.