Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
10.1051/0004-6361/201936214
3 Pith papers cite this work. Polarity classification is still indexing.
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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.
Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.
citing papers explorer
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Energetic particle-mediated interplanetary shocks observed by Solar Orbiter
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
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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.
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Do Solar Energetic Electrons cross the Heliospheric Current Sheet? - A Statistical Study
Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.