Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code

Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code

We present a method of conducting data-driven simulations of solar active regions and flux emergence with the MURaM radiative magnetohydrodynamics (MHD) code. The horizontal electric field that is derived from the full velocity and magnetic vectors is implemented at the photospheric (bottom) boundar...

Full description

Bibliographic Details
Main Authors: Feng Chen, Mark C. M. Cheung, Matthias Rempel, Georgios Chintzoglou
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Radiative magnetohydrodynamics
Magnetohydrodynamical simulations
Solar magnetic flux emergence
Solar magnetic reconnection
Solar active regions
Solar flares
Online Access:https://doi.org/10.3847/1538-4357/acc8c5

Internet

https://doi.org/10.3847/1538-4357/acc8c5

Similar Items