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 7

a) Dependence of the number of shock waves (IP_n) as a function of R_d; b) Dependence of the time spent on passing a particular segment (length = 0.067 AU; T_s) as a function of R_d; N_{IP_Rd} is the ratio of IP_n on each segment (IP_s) to T_s as a function of R_d.

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