activity
20112024
most citedWhat Sustained Multi-Disciplinary Research Can Achieve: The Space Weather Modeling Framework

128 citations · 507 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2024

Interaction between a Coronal Mass Ejection and Comet 67P/Churyumov-Gerasimenko

Zhenguang Huang, Gabor Toth, Tamas I. Gombosi +6

The interaction between a Coronal Mass Ejection (CME) and a comet has been observed several times by in-situ observations from the Rosetta Plasma Consortium (RPC), which is designe…

astro-ph.SR2024

Adjusting the Potential Field Source Surface Height Based on MHD Simulations

Zhenguang Huang, Gabor Toth, Jia Huang +3

A potential field solution is widely used to extrapolate the coronal magnetic field above the Sun's surface to a certain height. This model applies the current-free approximation a…

astro-ph.SR2024

Solar Wind Driven from GONG Magnetograms in the Last Solar Cycle

Zhenguang Huang, Gabor Toth, Nishtha Sachdeva +1

In a previous study, Huang et al. (2023) used the Alfven Wave Solar atmosphere Model (AWSoM), one of the widely used solar wind models in the community, driven by ADAPT-GONG magnet…

astro-ph.SR2023

Solar Wind with Field Lines and Energetic Particles (SOFIE) Model: Application to Historical Solar Energetic Particle Events

Lulu Zhao, Igor Sokolov, Tamas Gombosi +7

In this paper, we demonstrate the applicability of the data-driven and self-consistent solar energetic particle model, Solar-wind with FIeld-lines and Energetic-particles (SOFIE),…

physics.space-ph2023★ 18 cited

Parker Solar Probe Observations of High Plasma Beta Solar Wind from Streamer Belt

Jia Huang, J. C. Kasper, Davin E. Larson +23

In general, slow solar wind from the streamer belt forms a high plasma beta equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely the heliospheric pl…

astro-ph.SR2022★ 11 cited

Solar wind modeling with the Alfven Wave Solar atmosphere Model driven by HMI-based Near-Real-Time maps by the National Solar Observatory

Nishtha Sachdeva, Ward B Manchester, Igor Sokolov +6

We explore model performance for the Alfven Wave Solar atmosphere Model (AWSoM) with near-real-time (NRT) synoptic maps of the photospheric vector magnetic field. These maps, produ…