Study on two Methods for Nonlinear Force-free Extrapolation Based on Semi-Analytical Field
arXiv:1405.2158 · doi:10.1007/s11207-010-9691-4
Abstract
In this paper, two semi-analytical solutions of force free fields (\citeauthor{low90}, \citeyear{low90}) have been used to test two nonlinear force-free extrapolation methods. One is the boundary integral equation (BIE) method developed by \citeauthor{yan00} (\citeyear{yan00}), and another is the approximate vertical integration (AVI) method developed by \citeauthor{son06} (\citeyear{son06}). Some improvements for the AVI method have been taken to avoid the singular points in the process of calculation. It is found that the correlation coefficients between the first semi-analytical field and extrapolated field by BIE, and also that by improved AVI, are greater than below a height 10 of the lower boundary. While for the second semi-analytical field, these correlation coefficients are greater than below the same relative height. Although the differences between the semi-analytical solutions and the extrapolated fields exist for both BIE and AVI methods, these two methods can give reliable results for the height of about 15 of the extent of the lower boundary.
19 pages, 11 figures. solar physics 2011
References in corpus (6)
- Optimization code with weighting function for the reconstruction of coronal magnetic fields
- Preprocessing of vector magnetograph data for a non-linear force-free magnetic field reconstruction
- A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
- Nonlinear force-free models for the solar corona I. Two active regions with very different structure
- How to use magnetic field information for coronal loop identification?
- Formation Heights of Extreme Ultraviolet Lines in an Active Region Derived by Correlation of Doppler Velocity and Magnetic Field
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