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From the 1 of 9 linked papers with an AI index.

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9 papers

astro-ph.SR2026

Energetic Particle Acceleration and Transport: Interplanetary Coronal Mass Ejections and Shocks

Olga E. Malandraki, Christina M. S. Cohen, Joe Giacalone +16

The paper reviews recent observations of solar energetic particles and how interplanetary coronal mass ejections and shocks accelerate and transport these particles, highlighting d…

astro-ph.SR2026

Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter

Xiaohang Chen, Gang Li, Joe Giacalone +12

The propagation of solar energetic particles (SEPs) through the heliosphere is primarily guided by the interplanetary magnetic field (IMF) which is embedded in the solar wind plasm…

physics.space-ph2026

Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023

Malik H. Walker, Robert C. Allen, George C. Ho +6

During the propagation of interplanetary coronal mass ejections (ICMEs), evolution of the ICME-driven shock along with interactions with other solar wind structures, planetary bodi…

physics.space-ph2026

Sunward Streaming 3He-rich SEP Events Observed by Solar Orbiter and Parker Solar Probe during Perihelion Passage

Samuel T. Hart, George C. Ho, Michael R. Terres +7

We report on two 3He-rich solar energetic particle (SEP) events observed by Solar Orbiter (SO) and Parker Solar Probe (PSP) during the April 1 - 4, 2024 conjunction when both space…

astro-ph.SR2025

Evidence of Time-Dependent Diffusive Shock Acceleration in the 2022 September 5 Solar Energetic Particle Event

Xiaohang Chen, Lulu Zhao, Joe Giacalone +15

On 2022 September 5, a large solar energetic particle (SEP) event was detected by Parker Solar Probe (PSP) and Solar Orbiter (SolO), at heliocentric distances of 0.07 and 0.71 au,…

astro-ph.SR2025

Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter

Xiaomin Chen, Chuan Li, Zigong Xu +5

Local particle acceleration in the shock sheath region formed during the interaction between multiple coronal mass ejections (CMEs) is a complicated process that is still under inv…