Poster abstract details

The introduction of rotation and magnetic field in stellar evolution codes is necessary to reproduce most of the seismic indicators that we already registered. But their implementation is difficult and new questions emerge on young stellar dynamos and on boundary conditions. So this theoretical effort calls for complementary measurements in order to separate properly the role of the different processes.
After a rapid description of where we are on the theoretical side, we shall show how the coming missions like PICARD and ASPIICS and new instruments like GOLF-NG can contribute to give a more global view of the Sun with evident consequences (that we shall consider) on Stars and Planets interaction.