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Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions

  • Authors: Lucas A. Tarr, N. Dylan Kee, Mark G. Linton, Peter W. Schuck, James E. Leake

Lucas A. Tarr et al 2024 The Astrophysical Journal Supplement Series 270 .

  • Provider: AAS Journals

Caption: Figure 11.

Comparison between a potential field extrapolation (left column), the result of data driving using a driving cadence of Δt = 20δt (center column), and a nonlinear force free field extrapolation using the optimization code provided by Thomas Wiegelmann (right). The top and bottom rows show two different perspectives. The extrapolation time t = 1.55t N is at courant step 380, near the end of the spheromak’s expansion.

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