Energetic particle acceleration and transport with the novel Icarus + PARADISE model | Journal of Space Weather and Space Climate

Topical Issue - CMEs, ICMEs, SEPs: Observational, Modelling, and Forecasting Advances

Open Access

Figure 3

Plots of the magnetic field magnitude (top panel), the solar wind speed (middle panel), and the solar wind particle number density (bottom panel) versus longitude ϕ at radial distance r = 1 au and colatitude θ = 90° obtained by Icarus (blue solid line) and EUHFORIA (red dashed line).

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