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Bipolar Jets Launched by a Mean-field Accretion Disk Dynamo

  • Authors: Christian Fendt, and Dennis Gaßmann

2018 The Astrophysical Journal 855 130.

  • Provider: AAS Journals

Caption: Figure 16.

Ratio of the toroidal to poloidal magnetic field strength (colors) and poloidal magnetic flux surfaces (lines) for simulation run Dt103 with ﹩{\alpha }_{0}=-0.005﹩ at time 10,000. The dashed gray lines indicate a different polarity of the magnetic field.

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