Fig. 3.

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Magnetic field magnitude and components, solar wind speed, proton number density, and proton temperature vs. time in the 3-h time window centered at the shock arrival time. The shock arrival time (∼22:30 UT) is marked by the dashed magenta line. The red and blue shaded areas denote the shortest (dark) and largest (light) averaging windows used for the shock parameter estimation upstream and downstream, respectively.
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