The Alfven wave travels at 44.6 km/s, which is 0.015% of the speed of light.
Plasma beta is 1.01e-7: the magnetic field dominates thermal pressure by a large margin. This is the low-beta regime common in the solar corona and tokamaks.
The plasma flow is super-Alfvenic with Alfven Mach number M_A = 11.210.
Ion inertial length is 9.31 m. At scales smaller than this, the Hall effect becomes important and the simple MHD approximation breaks down.
Next stepCompare the Alfven velocity to your flow speed to determine whether Alfven waves can propagate upstream against the flow.