activity
20042021
most citedWhat Sustained Multi-Disciplinary Research Can Achieve: The Space Weather Modeling Framework

128 citations · 158 across the 2 of their papers we have counts for

collaborators

9 papers

physics.space-ph2021128 cited

What Sustained Multi-Disciplinary Research Can Achieve: The Space Weather Modeling Framework

Tamas I. Gombosi, Yuxi Chen, Alex Glocer +15

MHD-based global space weather models have mostly been developed and maintained at academic institutions. While the "free spirit" approach of academia enables the rapid emergence a…

astro-ph.SR2020

Predicting solar flares with machine learning: investigating solar cycle dependence

Xiantong Wang, Yang Chen, Gabor Toth +7

A deep learning network, Long-Short Term Memory (LSTM) network, is used in this work to predict whether the maximum flare class an active region (AR) will produce in the next 24 ho…

astro-ph.SR2019

Interpreting LSTM Prediction on Solar Flare Eruption with Time-series Clustering

Hu Sun, Ward Manchester, Zhenbang Jiao +2

We conduct a post hoc analysis of solar flare predictions made by a Long Short Term Memory (LSTM) model employing data in the form of Space-weather HMI Active Region Patches (SHARP…

astro-ph.SR2019

Solar Flare Intensity Prediction with Machine Learning Models

Zhenbang Jiao, Hu Sun, Xiantong Wang +4

We develop a mixed Long Short Term Memory (LSTM) regression model to predict the maximum solar flare intensity within a 24-hour time window 024, 630, 1236 and 24$…

astro-ph.SR2019

Identifying Solar Flare Precursors Using Time Series of SDO/HMI Images and SHARP Parameters

Yang Chen, Ward B. Manchester, Alfred O. Hero +7

We present several methods towards construction of precursors, which show great promise towards early predictions, of solar flare events in this paper. A data pre-processing pipeli…

astro-ph.SR2018

Extended MHD modeling of the steady solar corona and the solar wind

Tamas I. Gombosi, Bart van der Holst, Ward B. Manchester +1

The history and present state of large-scale magnetohydrodynamic (MHD) modeling of the solar corona and the solar wind with steady or quasi-steady coronal physics is reviewed. We p…