3 papers
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),…