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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 .

Caption: Figure 12.

Same as Figure 11, but including field lines initiated near the edge of the emerged portion of the spheromak.