An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data

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	An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data
	Hayashi, Keiji; Feng, Xueshang; Xiong, Ming; Jiang, Chaowei; Hayashi, K (reprint author), Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, SIGMA Weather Grp, Beijing 100190, Peoples R China.; Hayashi, K (reprint author), Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi 4648601, Japan.
作者部门	空间科学部
发表期刊	ASTROPHYSICAL JOURNAL
	2018
卷号	855 期号:1 页码:11
ISSN	0004-637X
语种	英语
关键词	Magnetohydrodynamics (Mhd) Sun: Magnetic Fields Sunspots
摘要	For realistic magnetohydrodynamics (MHD) simulation of the solar active region (AR), two types of capabilities are required. The first is the capability to calculate the bottom-boundary electric field vector, with which the observed magnetic field can be reconstructed through the induction equation. The second is a proper boundary treatment to limit the size of the sub-Alfvenic simulation region. We developed (1) a practical inversion method to yield the solar-surface electric field vector from the temporal evolution of the three components of magnetic field data maps, and (2) a characteristic-based free boundary treatment for the top and side sub-Alfvenic boundary surfaces. We simulate the temporal evolution of AR 11158 over 16 hr for testing, using Solar Dynamics Observatory/Helioseismic Magnetic Imager vector magnetic field observation data and our time-dependent three-dimensional MHD simulation with these two features. Despite several assumptions in calculating the electric field and compromises for mitigating computational difficulties at the very low beta regime, several features of the AR were reasonably retrieved, such as twisting field structures, energy accumulation comparable to an X-class flare, and sudden changes at the time of the X-flare. The present MHD model can be a first step toward more realistic modeling of AR in the future.
收录类别	SCI
文献类型	期刊论文
条目标识符	http://ir.nssc.ac.cn/handle/122/6193
专题	空间科学部
通讯作者	Hayashi, K (reprint author), Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, SIGMA Weather Grp, Beijing 100190, Peoples R China.; Hayashi, K (reprint author), Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi 4648601, Japan.
推荐引用方式 GB/T 7714	Hayashi, Keiji,Feng, Xueshang,Xiong, Ming,et al. An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data[J]. ASTROPHYSICAL JOURNAL,2018,855(1):11.
APA	Hayashi, Keiji,Feng, Xueshang,Xiong, Ming,Jiang, Chaowei,Hayashi, K ,&Hayashi, K .(2018).An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data.ASTROPHYSICAL JOURNAL,855(1),11.
MLA	Hayashi, Keiji,et al."An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data".ASTROPHYSICAL JOURNAL 855.1(2018):11.

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2018855111.pdf（4694KB）	期刊论文	作者接受稿	开放获取	CC BY-NC-SA	请求全文