Fig. A.2

Variation of a: radius, b: density ρ, and c: poloidal and toroidal magnetic field (in solid and dashed curves respectively) along a magnetic wind surface as a function of z∕r0, for the four computed MHD DW solutions. The Alfvén point for each solution is plotted as a filled dot. Quantities are normalized by the mid-plane value of radius, density, and vertical magnetic field Bz,0 at r0. The latter are related to the dimensional parameters of the system through
and
, where ms ≃ 1−2 is the Mach number of the accretion flow (Combet & Ferreira 2008).
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