Abstract
The stationary axisymmetric outflow from a rotating sphere with a (split) monopole magnetic field is considered. The stream equation describing the outflow is linearized in terms of the Michel magnetization parameter σ-1 ≪ 1, which allows a self-consistent analysis of the direct problem. It is shown that for a finite σ the fast magnetosonic surface is located at a finite distance ∼σ1/3RL (RL = c/ΩF is the light cylinder). We have also found that the particle energy at the fast surface is just equal to the Michel value γ ∼ σ1/3. The particle acceleration and magnetic field collimation are shown to become ineffective outside the fast magnetosonic surface.
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Beskin, V. S., Kuznetsova, I. V., & Rafikov, R. R. (1998). On the MHD effects on the force-free monopole outflow. Monthly Notices of the Royal Astronomical Society, 299(2), 341–348. https://doi.org/10.1046/j.1365-8711.1998.01659.x
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