中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Non-equilibrium Ionization Effects on Extreme-ultraviolet Emissions Modulated by Standing Sausage Modes in Coronal Loops

文献类型:期刊论文

作者Shi, Mijie1,2; Li, Bo1; Van Doorsselaere, Tom3; Chen, Shao-Xia1; Huang, Zhenghua1
刊名ASTROPHYSICAL JOURNAL
出版日期2019-01-10
卷号870期号:2页码:10
关键词magnetohydrodynamics (MHD) Sun: corona Sun: UV radiation waves
ISSN号0004-637X
DOI10.3847/1538-4357/aaf393
英文摘要Forward-modeling the emission properties in various passbands is important for confidently identifying magnetohydrodynamic waves in the structured solar corona. We examine how non-equilibrium ionization (NEI) affects the extreme-ultraviolet (EUV) emissions modulated by standing fast sausage modes (FSMs) in coronal loops, taking the Fe IX 171 angstrom and Fe XII 193 angstrom emission lines as examples. Starting with the expressions for linear FSMs in straight cylinders, we synthesize the specific intensities and spectral profiles for the two spectral lines by incorporating the self-consistently derived ionic fractions in the relevant contribution functions. We find that relative to the case where equilibrium ionization (EI) is assumed, NEI considerably impacts the intensity modulations, but shows essentially no effect on the Doppler velocities or widths. Furthermore, NEI may affect the phase difference between intensity variations and those in Doppler widths for Fe XII 193 angstrom when the line of sight is oblique to the loop axis. While this difference is 180 degrees when EI is assumed, it is similar to 90 degrees when NEI is incorporated for the parameters we choose. We conclude that in addition to viewing angles and instrumental resolutions, NEI further complicates the detection of FSMs in spectroscopic measurements of coronal loops in the EUV passband.
WOS关键词OSCILLATIONS ; PULSATIONS ; WAVES ; PROPAGATION ; EUV
资助项目National Natural Science Foundation of China[41474149] ; National Natural Science Foundation of China[41604145] ; National Natural Science Foundation of China[41674172] ; National Natural Science Foundation of China[11761141002] ; KU Leuven[GOA-2015-014] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme[724326] ; Young Scholar Program of Shandong University Weihai[2017WHWLJH07] ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China[KLSA201801]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000455931200004
出版者IOP PUBLISHING LTD
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; KU Leuven ; KU Leuven ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; Young Scholar Program of Shandong University Weihai ; Young Scholar Program of Shandong University Weihai ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; KU Leuven ; KU Leuven ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; Young Scholar Program of Shandong University Weihai ; Young Scholar Program of Shandong University Weihai ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; KU Leuven ; KU Leuven ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; Young Scholar Program of Shandong University Weihai ; Young Scholar Program of Shandong University Weihai ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; KU Leuven ; KU Leuven ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; Young Scholar Program of Shandong University Weihai ; Young Scholar Program of Shandong University Weihai ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China ; Open Research Program of the Key Laboratory of Solar Activity of National Astronomical Observatories of China
源URL[http://ir.bao.ac.cn/handle/114a11/24652]  
专题中国科学院国家天文台
通讯作者Li, Bo
作者单位1.Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Inst Space Sci, Weihai 264209, Peoples R China
2.Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100012, Peoples R China
3.Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B, B-3001 Leuven, Belgium
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GB/T 7714
Shi, Mijie,Li, Bo,Van Doorsselaere, Tom,et al. Non-equilibrium Ionization Effects on Extreme-ultraviolet Emissions Modulated by Standing Sausage Modes in Coronal Loops[J]. ASTROPHYSICAL JOURNAL,2019,870(2):10.
APA Shi, Mijie,Li, Bo,Van Doorsselaere, Tom,Chen, Shao-Xia,&Huang, Zhenghua.(2019).Non-equilibrium Ionization Effects on Extreme-ultraviolet Emissions Modulated by Standing Sausage Modes in Coronal Loops.ASTROPHYSICAL JOURNAL,870(2),10.
MLA Shi, Mijie,et al."Non-equilibrium Ionization Effects on Extreme-ultraviolet Emissions Modulated by Standing Sausage Modes in Coronal Loops".ASTROPHYSICAL JOURNAL 870.2(2019):10.

入库方式: OAI收割

来源:国家天文台

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