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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. 1.

Radial and θ velocity components and the plasma density as functions of θ at fixed radius at (a) ﹩\Delta \Phi =0.5﹩, 1.0, and 1.5 and (b) ﹩\Delta \Phi =1.5﹩, 2.0. These plots are for the ﹩n=1﹩ self‐similar field configuration with a uniform initial density distribution (﹩p=0﹩). Time is measured in units of ﹩1/ \Delta \Omega ﹩. The critical twist angle ﹩\Delta \Phi _{c}﹩ is attained at ﹩t_{c}=2.036﹩.

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