6 citations · 6 across the 6 of their papers we have counts for
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Evolution of Coronal Mass Ejections in Different Data-Driven Solar Wind Conditions
Nishtha Sachdeva, Zhenguang Huang, Gabor Toth +3
Numerical models of the solar wind and coronal mass ejections (CMEs) utilize photospheric magnetic field observations to prescribe the inner boundary conditions for the plasma solu…
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,…
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…
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…
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),…