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In this paper, we demonstrate the applicability of the data-driven andself-consistent solar energetic particle model, Solar-wind with FIeld-lines andEnergetic-particles (SOFIE), to simulate acceleration and transport processesof solar energetic particles. SOFIE model is built upon the Space WeatherModeling Framework (SWMF) developed at the University of Michigan. In SOFIE,the background solar wind plasma in the solar corona and interplanetary spaceis calculated by the Aflv\'en Wave Solar-atmosphere Model(-Realtime) (AWSoM-R)driven by the near-real-time hourly updated Global Oscillation Network Group(GONG) solar magnetograms. In the background solar wind, coronal mass ejections(CMEs) are launched by placing an imbalanced magnetic flux rope on top of theparent active region, using the Eruptive Event Generator using Gibson-Low model(EEGGL). The acceleration and transport processes are modeled by theMultiple-Field-Line Advection Model for Particle Acceleration (M-FLAMPA). Inthis work, nine solar energetic particle events (Solar Heliospheric andINterplanetary Environment (SHINE) challenge/campaign events) are modeled. Thethree modules in SOFIE are validated and evaluated by comparing withobservations, including the steady-state background solar wind properties, thewhite-light image of the CME, and the flux of solar energetic protons, atenergies of > 10 MeV.

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