Our research group focuses on advanced studies in fluid dynamics, addressing key challenges in areas such as fluid turbulence, stratified fluid fields, hydrodynamic stability, and the collective behavior of traveling waves in sheared flows. We also conduct cutting-edge numerical and laboratory simulations of hypersonic jets, along with pioneering efforts in astrophysics—specifically, mid-term stellar jet simulations in laboratory settings and the analysis of solar wind data and related magnetic fields.

Our research has wide-ranging applications, including subgrid-scale modeling (LES, SGS), turbulent mixing, cloud-clear air interface dynamics, energy transport by traveling waves in microchannels, and studies on wall and wake flows, under-expanded jets, and astrophysical jet collimation under partial physical similitude in Earth-based laboratories.

In collaboration with several national and international partners, we are pushing the boundaries of fluid dynamics and astrophysical research. Our group is based in the Department of APPLIED SCIENCE AND TECHNOLOGY (DISAT) at Politecnico di Torino, where we have developed several in-house computational fluid dynamics (CFD) codes. These codes are available for Open Access on our website, with our recently updated Software Download pages now fully operational.