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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 9.

Time–distance plot showing the horizontal expansion of the spheromak along the x-direction along the line (y = 0, z b  = 1.11) for four primitive variables: (a) ρ, (b) B z , (c) v x , and (d) v y . The approximate average expansion rate of ﹩{dx}/{dt}\approx 2/1.4\left[{L}_{N}/{T}_{N}\right]﹩ is indicated by the white dashed line.

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