A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2021; you can also visit the original URL.
The file type is application/pdf
.
MHD Modeling of Solar Coronal Magnetic Evolution Driven by Photospheric Flow
2021
Frontiers in Physics
It is well-known that magnetic fields dominate the dynamics in the solar corona, and new generation of numerical modeling of the evolution of coronal magnetic fields, as featured with boundary conditions driven directly by observation data, are being developed. This paper describes a new approach of data-driven magnetohydrodynamic (MHD) simulation of solar active region (AR) magnetic field evolution, which is for the first time that a data-driven full-MHD model utilizes directly the
doi:10.3389/fphy.2021.646750
fatcat:vdar4pj5i5c7ferqaupnoqku24