building on my recent advances in the field of rotating and magnetohydrodynamic turbulence
, I will derive a set of reduced equations to simulate such turbulent flows in the vicinity of the transition where bulk 3d waves appear on a 2d turbulent flow.
This suggests that there is a universal basic property governing the evolution of magnetohydrodynamic turbulence
over finite distances - in this case a finite distance of over 200 million miles.
Other topics include magnetohydrodynamic turbulence
at low magnetic Reynolds number, sea ice rheology, the effects of wind on plants, horizontal convection, blood flow in end-to-side anastomoses, and inertial cavitation for drug delivery and noninvasive therapy.