The soft X-ray Neupert effect as a proxy for solar energetic particle injection - A proof-of-concept physics-based forecasting model | Journal of Space Weather and Space Climate

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Fig. 3

Simulated temporal evolution of the differential intensity for a range of radial mean free path (λ_r) values as indicated in the legend. Note that the model takes ~5 h to settle into a quasi-steady state (indicated by the grey shading) if initialised with constant SEP injection at the inner boundary.

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