Evolution of Jupiter’s magnetosphere under different solar wind conditions. (top) North-south component of the magnetic field (B_z, positive northward), plasma number density, radial flow (V_r, positive outflow), and azimuthal flow (V_ϕ, positive anticlockwise) at the equatorial plane of Jupiter’s magnetosphere during at 437 : 00 simulation time (ST) from the GAMERA. (bottom) Solar wind ram pressure conditions driving the GAMERA. Movie A1 shows the evolution during 380 : 00–500 : 00 ST. The movie is available online.