Theoretical profiles of magnetic field components are obtained by advancing a torus at a speed of 600 km s⁻¹ through three virtual satellites. The first column presents an isosurface Ψ = 1 for the Soloviev solution, with three torus inclinations: ω = 0° (top panel), ω = 45° (middle panel), and ω = −45° (bottom panel). The second column represents, for these three configurations, the evolution of magnetic field components (in GSE) at the level of a virtual satellite (blue) placed directly in the direction of torus propagation. The third column corresponds to the passage through the offset virtual satellite (orange) at an angle ϕ = 10° relative to the propagation direction. The fourth column corresponds to the offset green satellite at an angle ϕ = −10°. The dashed lines correspond to the magnetic field components obtained from the Soloviev CME model, whereas the solid lines correspond to the mMT solution.