activity
20232026
most citedTransfer of Entropy between the Magnetic Field and Solar Energetic Particles during an Interplanetary Coronal Mass Ejection

6 citations · 7 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026★ 1 cited

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

Predicting Associations between Solar Flares and Coronal Mass Ejections Using SDO/HMI Magnetograms and a Hybrid Neural Network

Jialiang Li, Vasyl Yurchyshyn, Jason T. L. Wang +6

Solar eruptions, including flares and coronal mass ejections (CMEs), have a significant impact on Earth. Some flares are associated with CMEs, and some flares are not. The associat…

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★ 6 cited

Transfer of Entropy between the Magnetic Field and Solar Energetic Particles during an Interplanetary Coronal Mass Ejection

M. E. Cuesta, G. Livadiotis, D. J. McComas +4

Thermodynamics of solar wind bulk plasma have been routinely measured and quantified, unlike those of solar energetic particles (SEPs), whose thermodynamic properties have remained…

astro-ph.SR2025

Prediction of Halo Coronal Mass Ejections Using SDO/HMI Vector Magnetic Data Products and a Transformer Model

Hongyang Zhang, Ju Jing, Jason T. L. Wang +6

We present a transformer model, named DeepHalo, to predict the occurrence of halo coronal mass ejections (CMEs). Our model takes as input an active region (AR) and a profile, where…

astro-ph.SR2025

Comparing Methods for Calculating Solar Energetic Particle Intensities: Re-binning versus Spectral Binning

M. E. Cuesta, L. Y. Khoo, G. Livadiotis +13

Solar energetic particle (SEP) events have been observed for decades in the interplanetary medium by spacecraft measuring the intensity of energetic ions and electrons. These inten…

cs.LG2025

Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning

Khalid A. Alobaid, Jason T. L. Wang, Haimin Wang +6

The application of machine learning to the study of coronal mass ejections (CMEs) and their impacts on Earth has seen significant growth recently. Understanding and forecasting CME…

astro-ph.SR2024

Observations of Kappa Distributions in Solar Energetic Protons and Derived Thermodynamic Properties

M. E. Cuesta, A. T. Cummings, G. Livadiotis +13

In this paper we model the high-energy tail of observed solar energetic proton energy distributions with a kappa distribution function. We employ a technique for deriving the therm…

astro-ph.SR2024

Kappa-tail technique: Modeling and application to Solar Energetic Particles observed by Parker Solar Probe

G. Livadiotis, A. T. Cummings, M. E. Cuesta +10

We develop the kappa-tail fitting technique, which analyzes observations of power-law tails of distributions and energy-flux spectra and connects them to theoretical modeling of ka…

physics.space-ph2023

A Machine Learning Approach to Understanding the Physical Properties of Magnetic Flux Ropes in the Solar Wind at 1 AU

Hameedullah Farooki, Yasser Abduallah, Sung Jun Noh +5

Interplanetary magnetic flux ropes (MFRs) are commonly observed structures in the solar wind, categorized as magnetic clouds (MCs) and small-scale MFRs (SMFRs) depending on whether…

physics.space-ph2023

A Closer Look at Small-Scale Magnetic Flux Ropes in the Solar Wind at 1 AU: Results from Improved Automated Detection

Hameedullah Farooki, Sung Jun Noh, Jeongwoo Lee +7

Small-scale interplanetary magnetic flux ropes (SMFRs) are similar to ICMEs in magnetic structure, but are smaller and do not exhibit ICME plasma signatures. We present a computati…