Global MHD Simulations of the Time-dependent Corona

We describe, test, and apply a technique to incorporate full-Sun, surface flux evolution into an MHD model of the global solar corona. Requiring only maps of the evolving surface flux, our method is similar to that of Lionello et al., but we introduce two ways to correct the electric field at the lo...

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Bibliographic Details
Main Authors: Roberto Lionello, Cooper Downs, Emily I. Mason, Jon A. Linker, Ronald M. Caplan, Pete Riley, Viacheslav S. Titov, Marc L. DeRosa
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad00be