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Toward a Quantitative Model for Simulation and Forecast of Solar Energetic Particle Production during Gradual Events. I. Magnetohydrodynamic Background Coupled to the SEP Model

  • Authors: D. Borovikov, I. V. Sokolov, I. I. Roussev, A. Taktakishvili, and T. I. Gombosi

2018 The Astrophysical Journal 864 88.

  • Provider: AAS Journals

Caption: Figure 3.

Simulated flux of SEP exceeding 10 MeV (GOES channel 2): along the extracted lines from the Sun to 1 au (top) and interpolated between footprints (small blue diamonds) of lines on a 1 au sphere (bottom).

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