Figure 2 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 2.

Three snapshots of a CME forming in the corona as seen from two angles in HGR: view onto a plane of 29.°5 latitude (top) and plane of 208.°5 longitude (bottom). Color shows the speed of the solar wind. Thin black lines are magnetic field lines extracted from the MHD solution and imported to the kinetic code.

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