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

We develop a general description of how information propagates through a magnetohydrodynamic (MHD) system based on the method of characteristics and use that to formulate numerical boundary conditions that are intrinsically consistent with the MHD equations. Our formulation includes two major advanc...

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Bibliographic Details

Published in:	The Astrophysical Journal Supplement Series
Main Authors:	Lucas A. Tarr, N. Dylan Kee, Mark G. Linton, Peter W. Schuck, James E. Leake
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Solar physics Solar magnetic fields Magnetohydrodynamical simulations Solar photosphere Solar corona Solar chromosphere
Online Access:	https://doi.org/10.3847/1538-4365/ad0e0c