Sketch of the geometry assumed in the model, not to scale. The ionized wind was modelled as a double-cone with a semi-opening angle of θ_w = 50.5° against which the ionized disk is placed in the intersected region between the disk wind and the boundary of the neutral disk, given by a double cone with a semi-opening angle of θ_a = 57° (Báez-Rubio et al. 2013). The electron density distribution assumed in the model depends on the radius as N_e ∝ r^-2.14. Within the ionized disk, at a radius of r_l, we placed eight symmetric regions depicted as spheres where the disk material is being ejected along the magnetic field lines. The conical helix depicts the trajectory followed by the material ejected from the disk from one of the regions.