Halo's Magnetic field as Evident from striated Interstellar Clouds (HOMERIC): Measuring the strength of the Galactic magnetic field in 3D through HI striations.

Magnetically regulated structure formation in molecular clouds: The role of the magnetic field and magnetohydrodynamic waves in the formation of the low density striations  (Read More) and high density elongated structures (filaments).

Modelling the dynamical and non-equilibrium chemical evolution of prestellar cores  (Read More).

Connecting the dynamics of molecular clouds with observations accounting for radiative transfer effects  (Read More).

Measurements of magnetic field strength through the Zeeman effect.

Modelling hydromagnetic processes in prestellar cores in the presence of ambipolar diffusion.