Jan Rybizki Title: Correlations between stellar dynamics and metallicity in the discs from a theorists perspective Abstract: The evolutionary disc model of Just and Jahreiss reproduces well the local kinematics of thick and thin disc. A simple chemical enrichment model is already included fitting the metallicity distribution of G dwarfs. Implications on the abundance distributions can be derived from this one-zone model. Radial gradients of metallicity, the alpha-enhancement and other element abundances combined with kinematic data can be determined with RAVE and SEGUE data. It is planned to include the enrichment of individual elements and later on to extend the model for different radii in order to determine the evolutionary timeline of star formation and the impact of radial mixing. This is work in progress and the current status will be presented.