Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2007/iii/paper-65/3/a/solution

Use a steady axisymmetric flow governed by ideal magnetohydrodynamics and take the Newtonian gravitational potential to be axisymmetric. Work locally on connected regular magnetic flux surfaces with nonzero poloidal flow. As usual for a wind without an imposed toroidal loop voltage, ; regularity on an included rotation axis guarantees this condition. It is needed to exclude steady cross-field flow in an annular domain.
Since , the poloidal magnetic flux function gives
The poloidal magnetic field is divergence-free. The zero toroidal electric field, with , gives . Define by . Steady mass conservation then gives
Thus is the magnetohydrodynamic mass loading, the mass flux per unit poloidal magnetic flux. Subtracting from the full velocity leaves only an azimuthal component. The cross product is
The steady ideal magnetohydrodynamic induction equation requires . Consequently the field-line angular velocity is and
Neither gas pressure nor axisymmetric gravity exerts an azimuthal torque. Multiplying the azimuthal momentum equation by combines the cylindrical curvature terms into angular-momentum transport:
Insert and use . It follows that
so the magnetohydrodynamic angular-momentum invariant is
The two terms account respectively for matter and Maxwell stress tensor transport of angular momentum.
Finally, subtracting times the logarithmic mass density equation from the logarithmic pressure equation gives . The specific entropy of a fixed-composition ideal gas is a function of . Steadiness and axisymmetry reduce its advection to . Hence
These flux-label functions are local on connected regular surfaces; disconnected components with the same numerical label need not share constants without an additional matching condition.

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