Study on Two Methods for Nonlinear Force-Free Extrapolation Based on Semi-Analytical Field

被引:12
|
作者
Liu, S. [1 ]
Zhang, H. Q. [1 ]
Su, J. T. [1 ]
Song, M. T. [2 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing, Peoples R China
[2] Chinese Acad Sci, Purple Mt Observ, Nanjing, Peoples R China
基金
中国国家自然科学基金;
关键词
Active regions; Magnetic fields; Photosphere; FREE MAGNETIC-FIELDS; NON-CONSTANT-ALPHA; 3-COMPONENT BOUNDARY-CONDITIONS; VECTOR MAGNETOGRAPH DATA; SOLAR CORONA; INTEGRAL-EQUATION; RECONSTRUCTION; SPACE; REPRESENTATION; COMPUTATION;
D O I
10.1007/s11207-010-9691-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, two semi-analytical solutions of force-free fields (Low and Lou, Astrophys. J. 352, 343, 1990) have been used to test two nonlinear force-free extrapolation methods. One is the boundary integral equation (BIE) method developed by Yan and Sakurai (Solar Phys. 195, 89, 2000), and the other is the approximate vertical integration (AVI) method developed by Song et al. (Astrophys. J. 649, 1084, 2006). Some improvements have been made to the AVI method 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 using the BIE method, and also that obtained by the improved AVI method, are greater than 90% below a height 10 of the 64 x 64 lower boundary. For the second semi-analytical field, these correlation coefficients are greater than 80% below the same relative height. Although differences between the semi-analytical solutions and the extrapolated fields exist for both the BIE and AVI methods, these two methods can give reliable results for heights of about 15% of the extent of the lower boundary.
引用
收藏
页码:41 / 57
页数:17
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