Using realistic models of the ionospheric conductivity and the field-aligned currents, we have determined how the distribution of the electric field in the polar cap ionosphere is controlled by the day-night contrast in conductivity and by the relative strengths of the region 1 and region 2 field-aligned currents. The sunward directed conductivity gradient act to set up a space charge in the polar cap which crowds the equipotentials toward and dawn sector for current sources of both region 1 and region 2 polarity; this effectively shifts the polar cap convection pattern toward dawn. Our results show further that for a given conductivity distribution the orientation of the electric field in the central polar cap depends sensitively on the relative strengths of the Birkeland currents pairs: for very weak region 2 currents (quiet times) the polar electric field is directed ?60¿ east of noon, for equal region 1 and 2 currents (disturbed times) the direction is ?10¿ est of noon, and for stronger region 2 than 1 currents (which may happen on occasion) the electric field points into the prenoon sector. These findings imply that the orientation of the polar cap electric field should serve as a measure or index of the ratio of region 1 to region 2 net current intensity and should possess correlations with geomagnetic activity similar to those of this ratio. This analysis does not include effects of possible source currents in the region of the polar cusp.