My primarily area of scientific research is space plasma turbulence. The closest natural laboratories of plasma are the solar wind and planetary magnetospheres, where in-situ measurements are possible at a very wide range of scales. For my research, I analyse in-situ satellite measurements of Cluster, Wind, Helios, STEREO, Ulysses in the solar wind and of Cluster, MMS and Cassini in the Earth’s and Saturn’s magnetospheres.