Members
magnetohydrodynamics; dynamo flows; flow stability and control; turbulence; numerical and reduced-order modelling of fluid flows
Extragalactic astrophysics, focussed on the study of galaxy clusters.
solar dynamo, solar wind, space weather, cosmic rays, stellar physics
Astrophysical magnetohydrodynamics, Galaxy formation and evolution
accretion models in AGNs, structure formation, cosmology
HPC simulations (MHD & PIC), semi-analytics
Particle acceleration, relativistic shocks and turbulence
Evolution of Binary Stars, MHD simulations, Formation and Destruction of Planets, Late stage planetary systems
Cosmic rays, magnetohydrodynamics, hydrodynamics, ISM, turbulence, magnetic fields
Interstellar turbulence, star formation, galactic magnetic fields
studies of MHD stability and current-dive in fusion plasmas, momentum transport from current-driven tearing and flow-driven magnetorotational instabilities, dynamo in magnetically and flow-dominated self-organized systems, and magnetic reconnection in fusion/laboratory and astrophysical plasmas.
MHD and Hall-MHD simulations of the plasma transport in space plasmas, particle acceleration and heating in magnetospheric boundary layers and solar wind, single and multi-spacecraft data-analysis techniques, statistical data analysis, machine learning and information theory.
Origin, impact, and observational properties of interstellar magnetic fields
Magnetosphere, Atmospheric erosion, Space climate
Solar Physics, in particular the propagation of magnetohydrodynamics waves in the solar atmosphere
Solar Physics, Plasma Physics, MHD simulations, Waves
Turbulent dynamo theory, Magnetic reconnection, Magneto-rotational instability - dynamo connection, computational astrophysics
Galaxy clusters, diffuse radio emission, particle acceleration, turbulence in the intracluster medium, primordial magnetic fields
HPC simulations, analytical
ICM: fluid instabilities, g-modes, multiphase gas formation, redshift evolution of multiphase gas.
energy transport via sound waves, thermal conduction (anisotropic in presence of B), viscous dissipation
Computational modelling related to Solar and Stellar Physics, Solar Dynamo, Solar Eruptions
Magnetic field amplification in weakly collisional plasmas, MHD and plasma physics, small-scale dynamo, turbulence
Cosmology: inflation, CMB, large scale structure formation, primordial magnetic fields;
Astrophysics: magnetohydrodynamic turbulence, magnetic reconnection
Observing and studying one of the major transient events, coronal mass ejections (CMEs) causing space weather. Specifically, studying and analysing solar origin of CMEs, their evolution in heliosphere, and assessing effects of CME interaction with surroundings using in-situ observations including recently launched spacecrafts like Parker Solar Probe, BepiColombo and Solar Orbiter, while CMEs propagate through interplanetary medium. To predict CME geoeffectiveness by completely constraining analytical model with remote observations.
