Modelling large solar proton events with the shock-and-particle model - Extraction of the characteristics of the MHD shock front at the cobpoint | Journal of Space Weather and Space Climate

Open Access

Fig. 6.

Top: Evolution of the injection rate of shock-accelerated protons at the cobpoint, Q, for a subset of modelled energy channels: left, for the 2000 April 4 SEP event and right for the 2006 December 13 SEP event. The bottom panels display the evolution of the VR parameter (see text for details).

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