Turbulent magnetic field in the H II region Sh 2โ27
Turbulent magnetic field in the H II region Sh 2โ27
Magnetic fields in the turbulent interstellar medium (ISM) are a key element in understanding Galactic dynamics, but there are many observational challenges. One useful probe for studying the magnetic field component parallel to the line of sight (LoS) is Faraday rotation of linearly polarized radio synchrotron emission, combined with H$\alpha$ โฆ