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Electric current density calculation and error analysis of solar active regions
Liang HF(梁红飞)1,2; Ma, L1; Zhao, HJ3; Xiang, FY4; Liang, HF (reprint author), Yunnan Normal Univ, Div Phys, Kunming 650011, Yunnan, Peoples R China.
Source PublicationNEW ASTRONOMY
2009-04
Volume14Issue:3Pages:294-301
DOI10.1016/j.newast.2008.09.002
Contribution Rank第2完成单位
Indexed BySCI
KeywordSun: Sunspots Sun: Vector Magnetic Field Electric Current Density
AbstractThis investigation centers upon calculating the vertical electric current densities from the two transverse components of vector magnetograms. The electric current density calculated by using the differential form of Ampere's law, j(z) = 1/mu(0) (del x B)(z), on the basis of spatially sampled transverse magnetic fields varies widely over an active region. In order to investigate how errors in the vector magnetograph measurements produce errors in the vertical electric current densities, we have numerically simulated the effects of random noise on a standard photospheric magnetic configuration produced by electric currents satisfying the force-free field conditions. We have also compared the results of the densities calculated by three different methods, and analyzed the reason inducing the differences in the results. The three methods are (1) to calculate the density using the differential form of Ampere's law j(z) = 1/mu(0) (del x B)(z); (2) to calculate the density using the integral form of Ampere's law along the square with edges at (x - Delta x, y - Delta y), (x + Delta x, y - Delta y), (x + Delta x, y + Delta y), (x - Delta x, y + Delta y) (hereafter small integral path) j(z) = (1/mu(0) closed integral(C1) B(t).dl)/dS; (3) to calculate the density by using the integral form of Ampere's law along the square with edges at (x - 2 Delta x, y - 2 Delta y), (x + 2 Delta x, y - 2 Delta y), (x + 2 Delta x, y + 2 Delta y), (x - 2 Delta x, y + 2 Delta y) (hereafter big integral path), j(z) = (1/mu(0) closed integral(C2) B(t).dl)/dS. It is found that the uncertainty of the measured electric current density increases along with the decreasing of the spatial pixel size ds. When the spatial pixel size of vector magnetograms is small enough, properly expanding the integral path can help us decrease the effect of random noise and demodulate the "true" electric current density from the measured transverse magnetograms. Close attention should be paid to the fact that some true fine-structure of the electric current density will be lost when the integral path exceeds the linear size of the smallest spatially resolved structure in the studied magnetogram. (C) 2008 Elsevier B.V. All rights reserved.
Funding OrganizationNSFC/Astronomy Associated Fund
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN1384-1076
URL查看原文
WOS IDWOS:000261990100011
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordVECTOR MAGNETOGRAPH DATA ; MAGNETIC-FIELD ; HELICITY ; ALPHA(AR) ; CORONA
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6143
Collection太阳物理研究组
Corresponding AuthorLiang, HF (reprint author), Yunnan Normal Univ, Div Phys, Kunming 650011, Yunnan, Peoples R China.
Affiliation1.Yunnan Normal University, Physics Division, Kunming 650011, Yunnan, China
2.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China
3.National Satellite Meteorological Center, China Meteorological Administration, Beijing 100081, China
4.Xiangtan University, Hunan, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Liang HF,Ma, L,Zhao, HJ,et al. Electric current density calculation and error analysis of solar active regions[J]. NEW ASTRONOMY,2009,14(3):294-301.
APA Liang HF,Ma, L,Zhao, HJ,Xiang, FY,&Liang, HF .(2009).Electric current density calculation and error analysis of solar active regions.NEW ASTRONOMY,14(3),294-301.
MLA Liang HF,et al."Electric current density calculation and error analysis of solar active regions".NEW ASTRONOMY 14.3(2009):294-301.
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