Testing magnetofrictional extrapolation with the Titov-Démoulin model of solar active regions

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Table 4:

Reconstruction accuracy of the Low_HFT equilibrium for different initial conditions.
Figure	Potential		Potential	Linear
of merit	Schmidt	TD_ex	Seehafer	Seehafer
$\sigma_J \times 10^{2}$	0.73	1.18	4.12	4.52
$\langle~\vert f_i\vert~\rangle \times 10^{5}$	6.90	11.98	16.18	14.47
$E_{\rm M}$	0.036	0.072	0.065	0.070
HFT apex	0.54%	1.05%	1.77%	2.06%
CFL apex	0.63%	4.11%	13.93%	17.99%
$\Phi$	1.10%	2.58%	2.26%	3.01%
$\tilde n$	3.89%	2.45%	17.54%	36.88%
$E_{\rm mag}$	0.37%	1.49%	2.30%	2.26%
$H_{\rm mag}$	4.43%	7.58%	1.38%	6.86%

Source LaTeX | All tables | In the text

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