Notes. IMF intensity of the simulation with the lowest |B_IMF| and the reconnection region located inside the computational domain (second and fourth columns). Maximum reconnection displacement in percent between the simulations with maximum and minimum |B_IMF| on the DS (NS) for Sun–Earth, Earth–Sun, and southward IMF orientations, for the North (South) pole for the northward orientation, and for West (East) of the magnetosphere for the ctr-cw ecliptic IMF orientation (third and fifth columns, respectively).