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Magnetically Linked Star‐Disk Systems. II. Effects of Plasma Inertia and Reconnection in the Magnetosphere

  • Authors: Dmitri A. Uzdensky, Arieh Königl, and C. Litwin

Uzdensky, Königl, & Litwin 2002 The Astrophysical Journal 565 1205.

  • Provider: AAS Journals

Caption: Fig. 3.

Ratio of the current density ﹩j_{\phi }﹩ to the plasma density ρ (in arbitrary units) as a function of θ for ﹩\Delta \Phi =0.5﹩, 1.0, and 1.5 in the ﹩n=1﹩ self‐similar model.

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