The density compression ratio of shock fronts associated with coronal mass ejections | Journal of Space Weather and Space Climate

Flares, coronal mass ejections and solar energetic particles and their space weather impacts

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Fig. 10

Mach numbers M_A (shaded regions) derived from the full ranges of X in Figure 9. Red lines indicate the critical Mach number for the determined θ_Bn. θ_Bn is also plotted by dashed lines (see the y-axes on the right-handed side).

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