Fig. 1.From: Kinetic effects on ion escape at Mars and Venus: Hybrid modeling studiesA HYB-Venus run to study the Venusian electromagnetic environment: (a) the total magnetic field, (b) the total electric field on the noon-midnight plane (y = 0). The solar wind flow is coming from the left. The spherical shell illustrates Venus. See Jarvinen et al. (2010b; Run 4), for the details of the run. The unit of the axes is the radius of Venus.Back to article page