Fig. 11From: Role of the solar wind magnetic field in the interaction of a non-magnetized body with the solar wind: An electromagnetic 2-D particle-in-cell simulation(a) The electron density ne and (b) the electric potential ϕ for the reduced Debye length case λD = 0.125Ro, obtained from the simulation run #3 at time t = 9.0 × 102ω-1 (180000 steps) when the solar wind flow has swept the simulation domain twice. The potential is normalized with .Back to article page