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From the 1 of 10 linked papers with an AI index.

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10 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…

physics.space-ph2026

Energetic particle-mediated interplanetary shocks observed by Solar Orbiter

D. Trotta, D. Lario, B. Reville +10

Context: In collisionless shocks, energetic particles can carry sufficient pressure to modify the upstream plasma and the shock structure itself, a regime often invoked in theories…

astro-ph.SR2026

Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption

Katharine K. Reeves, Daniel B. Seaton, Cynthia Cattell +20

We perform a detailed study of the energetics for a well-observed solar eruption and flare that occurred on 28 October 2021. This event included a GOES class X1.0 flare, a global E…

astro-ph.EP2026

Increased and Varied Radiation during the Sun's Encounters with Cold Clouds in the last 10 million years

Merav Opher, Joe Giacalone, Abraham Loeb +7

Recent research raises the possibility that 3 and 7 million years ago, the Sun encountered massive clouds that shrank the heliosphere--the solar cocoon protecting our solar system-…

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

Energy-dependent SEP Fe/O abundances during the May 2024 superstorm

G. D. Muro, C. M. S. Cohen, Z. Xu +16

During mid-May 2024, active region (AR) 13664 produced a series of M- and X-class flares along with several coronal mass ejections (CMEs) that resulted in exceptionally strong auro…