works on

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

activity
20242026
collaborators

9 papers

astro-ph.GA2026

Local Interstellar Flow Parameters from the First Intersection of IMAP-Lo's Parameter Tubes

Nathan A. Schwadron, Mitchell M. Shen, Fatemeh Rahmanifard +24

The Sun's motion through the interstellar medium creates a flow of interstellar neutral (ISN) atoms through the heliosphere. ISN He, due to its high universal abundance and relativ…

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

Review of Machine Learning Models for Solar Energetic Particle Prediction

Spiridon Kasapis, Pouya Hosseinzadeh, Kathryn Whitman +73

Solar energetic particle (SEP) events have attracted increasing attention due to their significant radiation hazards for aviation, spacecraft electronics, and human missions beyond…

astro-ph.SR2026

Parker Solar Probe observations of solar energetic particle (SEP) events with inverse velocity arrival (IVA) features

Zigong Xu, C. M. S. Cohen, R. A. Leske +21

In SEP events, velocity dispersion (VD) is characterized by the earlier arrival of faster, higher-energy particles relative to slower ones, assuming negligible acceleration time an…

astro-ph.SR2025

Energetic Particles from Quasi-Separatrix Layers and Current Sheets at the Sun

Nathan A. Schwadron, Ronald M. Caplan, Jon A. Linker +2

Quasi-separatrix layers (QSLs) at the Sun are created from regions where channels of open magnetic flux have footpoints near regions of large-scale closed magnetic flux. These regi…

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…