Statistical analysis of interplanetary shock waves measured by a Solar Wind Analyzer and a magnetometer onboard the Solar Orbiter mission in 2023 | Journal of Space Weather and Space Climate

Topical Issue - Fast and slow solar winds: Origin, evolution and Space Weather effects

Open Access

Figure 5

Distribution of the IP_n shock counts as functions θ_Bn (a) and β_us (b). Blue bins denote IP_n with θ_Bn < 45°, while red bins correspond to θ_Bn > 45°.

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