Research on astrophysical plasma is focused on investigating ionised matter that makes up most part of the visible universe. Plasma has a key role in dynamics and evolution of celestial bodies, ranging from stars and interestellar and intergalactic medium to the extreme conditions in surrounding areas of compact stars and black holes. This area combines theory, numerical simulations and observation to unravel its complex behaviour.

Main research topics/inquiries:

• • • Numerical modelling and observational analysis of coronal mass ejections, highlighting their crucial role in the dynamics of space weather.
    • Numerical simulations of eruptive processes in the solar atmosphere to understand particle acceleration and energy release mechanisms.
    • Study of dynamics, thermodynamics and radiative processes in high-temperature plasma, like plasma from galaxy clusters.
    • Investigation of mass accretion processes of compact objects, specifically black holes, focusing on the formation of accretion disks and the emission observed in multiple wavelengths.
    • Analysis of phenomena in turbulent galactic and intergalactic medium, including magnetic reconnection, particle acceleration, and conversion of magnetic energy into thermal and kinetic energy.
    

    
    Abilities/Strengths:

    This team has experience in numerical simulation of plasma using magnetohydrodynamic codes; moreover, the team has experience in the development of theoretical models that describe the behaviour of these systems. The team has a capacity to analyse observational data from diverse wavelengths, ranging from radio to X-ray wavelengths, allowing them to contrast theoretical models with astrophysical reality.