Extended Data Fig. 4: A 1D model of solar wind propagation surrounding the dates of the observations reported here.
From: Global upper-atmospheric heating on Jupiter by the polar aurorae
The orange shaded regions mark the period of ground-based observations. From top to bottom, each panel corresponds to solar wind density, temperature, radial (x; Jupiter–Sun line) and azimuthal (y; direction of planetary orbital motion) velocities, magnetic field By, dynamic pressure of the solar wind plotted linearly and logarithmically and the absolute magnetic field magnitude |B| (ref. 24). The 1σ uncertainty in arrival time of the solar wind at Jupiter is denoted by the horizontal, arrowed lines
