Multi-spacecraft and multi-instrument investigation of the solar wind properties

This talk reviews all recent results achieved in the investigation of solar wind properties using data from the Metis coronagraph aboard Solar Orbiter jointly with in-situ measurements acquired by Parker Solar Probe. Specifically, results on the propagation of the solar wind from the solar corona to the very inner heliosphere, the onset and evolution of turbulence, the link between the microphysical properties of the solar wind and the large-scale properties of the coronal source regions, the estimation of the rate of energy transfer by turbulence into the corona, and the energy budget in the corona will be presented. Finally, some possible future studies will be briefly discussed.