1984 Volume 53 Issue 5 Pages 1587-1589
The instability of the heterogeneous rotating flow in an azimuthal magnetic field is investigated for the flute-mode disturbance. Both the density ρ0 and the magnetic field intensity H0⁄r divided by the radial distance are assumed to have non-negative radial gradients. It is shown that the complex angular phase-velocity for any unstable flute-mode must lie within the semicircle in the upper half-plane which has
\sqrt(b−a)2−4(Va2⁄r2)m
for diameter. If the square of this expression is negative the rotating flow is stable. Here a and b are, respectively, the lower and the upper bound of angular velocity of the rotating flow, Va(r) is the Alfvén velocity and the suffix m means the minimum value.
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