Extended Data Fig. 5: A 1D model of solar wind propagation closely surrounding the dates of the observations reported here.
From: Global upper-atmospheric heating on Jupiter by the polar aurorae
The blue shaded regions mark the periods of ground-based observations. Absolute magnetic field magnitude |B| and dynamic pressure of the solar wind (SW) at Jupiter are shown as a function of date and time24. The 1σ uncertainty in arrival time of the solar wind at Jupiter is denoted by the horizontal arrowed lines.
