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Caption: Fig. 2.
Field‐line expansion caused by the relative rotation of the disk with respect to the star in the case of the ﹩n=0.5﹩ self‐similar model, where ﹩\Psi _{\mathrm{disk}\,}\sim r^{-n}﹩ (this figure is taken from Uzdensky et al. 2002a).
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