Fig. 7 from Simulation‐based Investigation of a Model for the Interaction between Stellar Magnetospheres and Circumstellar Accretion Disks

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Simulation‐based Investigation of a Model for the Interaction between Stellar Magnetospheres and Circumstellar Accretion Disks

Authors: Sean Matt, Anthony P. Goodson, Robert M. Winglee, and Karl-Heinz Böhm

Matt et al. 2002 The Astrophysical Journal 574 232.

Provider: AAS Journals

Caption: Fig. 7.

Snapshots from different times, early in the evolution of the baseline case, illustrating the rapid expansion of the poloidal magnetic field (solid lines). The gray scale is the logarithm of the number density measured in cm⁻³ (≤6.96 is white and ≥11.46 is black).

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