Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
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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Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023
Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
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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.