Figure 4 from Toward a Quantitative Model for Simulation and Forecast of Solar Energetic Particle Production during Gradual Events. I. Magnetohydrodynamic Background Coupled to the SEP Model

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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 4.

Time evolution of simulated flux of SEPs exceeding 10 MeV (GOES channel 2) at 1 au on a single line (solid black line) compared to GOES measurements (dashed black line). Time is measured from the CME initiation (4:00 on 2012 January 23).

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