For the same interplanetary shock seen at 0.8 and 1 AU, energetic particle profiles decorrelate with observer separation mainly at energies above 0.5 MeV, consistent with declining acceleration efficiency as the shock evolves.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.space-ph 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Variability in energetic particle observations at strong interplanetary shocks: Multi-spacecraft observations
For the same interplanetary shock seen at 0.8 and 1 AU, energetic particle profiles decorrelate with observer separation mainly at energies above 0.5 MeV, consistent with declining acceleration efficiency as the shock evolves.