Fig. 3

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Schematic depiction of the magnetospheric accretion and disk wind models. Shown here are the geometrical parameters defining each component. These are: the rotational axis Ω, the magnetic dipole axis μ, the magnetic obliquity βma, the wind focal point (S) displacement d, the inner and outer radius Rmi and Rmo, and width δRmag, of the magnetosphere, the inner and outer radius Rwi and Rwo, and width δRwind, of the wind, the dark disk radius Rdd beyond which the disk becomes completely opaque, and the cutoff zcrit at which the isothermal wind instantly reaches its 104 K temperature. The lower hemisphere parts of wind and magnetospheric funnel are omitted in this depiction for the sake of clarity.
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