Impact of dimensionless numbers on the efficiency of magnetorotational instability induced turbulent transport
Impact of dimensionless numbers on the efficiency of magnetorotational instability induced turbulent transport
The magnetorotational instability (MRI) is presently the most promising source of turbulent transport in accretion discs. However, some important issues still need to be addressed to quantify the role of MRI in discs; in particular no systematic investigation of the role of the physical dimensionless parameters of the problem on …