We present a new improved version of our force-free electrodynamics (FFE) numerical code in spherical coordinates that extrapolates the magnetic field in the inner solar corona from a photospheric vector magnetogram. The code satisfies the photospheric boundary condition and the condition divB=0 to machine accuracy. The performance of our method is evaluated with standard convergence parameters, and is found to be comparable to that of other nonlinear force-free extrapolations.
Cite
@article{arxiv.1209.5211,
title = {The Force-Free Electrodynamics Method for the Extrapolation of Coronal Magnetic Fields from Vector Magnetograms},
author = {Ioannis Contopoulos},
journal= {arXiv preprint arXiv:1209.5211},
year = {2015}
}
Comments
9 pages, 1 figure, accepted for publication in Solar Physics