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Fig. 1

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Magnetic field and radial speed v r (km/s) for the steady state solar wind solution. The left is on the meridional plane of ϕ = 180°−0° from 1 R s to 20 R s , the right is on the equatorial plane from 20 R s to 220 R s . The color contours represent the radial speed and streamlines denote the magnetic field lines.

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