Hybrid simulation results for the D182 orbit in the planes perpendicular to those shown in Fig. 9. Panels a–d: for the inbound and panels e–h: for the outbound IMF conditions. The cuts are in the yz-plane panels a,b,e and f: at x = +1.0R_M, and panels c,d,g and h: at x = –1.5 R_M. Panels a,c,d and e: magnitude of the magnetic field in logarithmic scale. Panels b,d,f and h: plasma flux normalized to the upstream solar wind flux Γ_sw = 1.15 × 10¹³ m⁻²⋅s. The solar wind flows into the planes shown here with 50 km s⁻¹ along the +y axis and the direction of the IMF in the yz-plane are shown by black arrows in panels a and e.