In this article, a method for obtaining the interface recombination velocity in a solar cell from a measurement of the dark curve is presented. The front interface recombination S f between window and emitter of a GaAs-InGaP heterojunction cell passivated by an AlInP window is used to demonstrate the method. By choosing a proper emitter thickness, the equation for the dark saturation current J 01 reduces to two terms, one related to the bulk recombination and the other to the interface recombination. The growth direction (either upright or inverted) is found to have a huge influence on S f as a result of the formation of an interfacial layer in the inverted grown cells. It is also shown that S f and, therefore, the optimum cell design strongly depend on the emitter doping level. Using the obtained S f data, an optimized cell configuration on the substrate and in a thin film has been calculated, leading to a 1% (absolute).