RECONSTRUCTION OF THE CORONAL MAGNETIC FIELD USING THE CESE-MHD METHOD | |
Jiang, Chaowei; Feng, Xueshang; Fan, Yuliang; Xiang, Changqing; Jiang, CW (reprint author), Chinese Acad Sci, Ctr Space Sci & Appl Res, State Key Lab Space Weather, SIGMA Weather Grp, Beijing 100190, Peoples R China. | |
Department | 空间科学部 |
Source Publication | ASTROPHYSICAL JOURNAL
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2011 | |
Volume | 727Issue:2Pages:101 |
ISSN | 0004-637X |
Language | 英语 |
Keyword | Magnetic Fields Magnetohydrodynamics (Mhd) Methods: Numerical Sun: Corona |
Abstract | We present a new implementation of the MHD relaxation method for reconstruction of the nearly force-free coronal magnetic field from a photospheric vector magnetogram. A new numerical MHD scheme is proposed to solve the full MHD equations by using the spacetime conservation-element and solution-element method. The bottom boundary condition is prescribed in a similar way as in the stress-and-relax method, by changing the transverse field incrementally to match the magnetogram, and other boundaries of the computational box are set by the nonreflecting boundary conditions. Applications to the well-known benchmarks for nonlinear force-free-field reconstruction, the Low & Lou force-free equilibria, validate the method and confirm its capability for future practical application, with observed magnetograms as inputs.; We present a new implementation of the MHD relaxation method for reconstruction of the nearly force-free coronal magnetic field from a photospheric vector magnetogram. A new numerical MHD scheme is proposed to solve the full MHD equations by using the spacetime conservation-element and solution-element method. The bottom boundary condition is prescribed in a similar way as in the stress-and-relax method, by changing the transverse field incrementally to match the magnetogram, and other boundaries of the computational box are set by the nonreflecting boundary conditions. Applications to the well-known benchmarks for nonlinear force-free-field reconstruction, the Low & Lou force-free equilibria, validate the method and confirm its capability for future practical application, with observed magnetograms as inputs. |
Indexed By | SCI |
Funding Project | 中国科学院空间科学与应用研究中心 |
Document Type | 期刊论文 |
Identifier | http://ir.nssc.ac.cn/handle/122/3248 |
Collection | 空间科学部 |
Corresponding Author | Jiang, CW (reprint author), Chinese Acad Sci, Ctr Space Sci & Appl Res, State Key Lab Space Weather, SIGMA Weather Grp, Beijing 100190, Peoples R China. |
Recommended Citation GB/T 7714 | Jiang, Chaowei,Feng, Xueshang,Fan, Yuliang,et al. RECONSTRUCTION OF THE CORONAL MAGNETIC FIELD USING THE CESE-MHD METHOD[J]. ASTROPHYSICAL JOURNAL,2011,727(2):101. |
APA | Jiang, Chaowei,Feng, Xueshang,Fan, Yuliang,Xiang, Changqing,&Jiang, CW .(2011).RECONSTRUCTION OF THE CORONAL MAGNETIC FIELD USING THE CESE-MHD METHOD.ASTROPHYSICAL JOURNAL,727(2),101. |
MLA | Jiang, Chaowei,et al."RECONSTRUCTION OF THE CORONAL MAGNETIC FIELD USING THE CESE-MHD METHOD".ASTROPHYSICAL JOURNAL 727.2(2011):101. |
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