Radiation non-ideal MHD simulations of protoplanetary disks
The movie shows density fluctuations of radiation non-ideal MHD simulations including dust sublimation (Flock et al. 2017).
Radiation MHD simulations
The movie shows the turbulent and thermal evolution of a protoplanetary disk using radiation MHD simulations including irradiation by the star. This simulations use real physical units. Turbulent velocities are presented in units of m/s.
It ranges from several thousand meters per second in the upper layers of the disk down to 10-100 meters per second in the midplane region. For more information please refer to Flock et al. 2013.
