Inverse velocity arrival in solar energetic particle events results from magnetic connectivity shifting from weak flanks to stronger apex regions of evolving CME-driven shocks.
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Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
citing papers explorer
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Shock properties for solar energetic particle events with signatures of inverse velocity arrival
Inverse velocity arrival in solar energetic particle events results from magnetic connectivity shifting from weak flanks to stronger apex regions of evolving CME-driven shocks.
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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.