The nature of MHD turbulence is shaped by means of energy injection on large scales, damping on small scales as well as environmental factors. New diagnostics are being developed for tracing the plasma properties of interstellar turbulence in conjunction with MHD and PIC simulations.
Astrophysical Magnetic fields as glue of astrophysical plasma, magnetic field is out of question one of the key properties that we want to know.
We investigate various ways to detect magnetic fields and their dynamics (turbulence), in particular, in the diffuse media.
Dust grain is one of the key components in interstellar medium.
They are intimately linked to the magnetic field and plasma as charge carriers in addition to their major rules in metallically and light propagation. All those are much determined by their dynamics, which we investigate.
We are investigating physical processes in space plasma, where rich information can be revealed by the measurement directly from various space probes, including the recently launched “Parker space probe". In particular, we are analysing the MHD perturbations, particle transport and plasma instabilities. Here is a representative plot with caption: