中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
NUMERICAL SIMULATION OF FAST-MODE MAGNETOSONIC WAVES EXCITED BY PLASMOID EJECTIONS IN THE SOLAR CORONA

文献类型:期刊论文

作者Yang, Liping; Zhang, Lei; He, Jiansen; Peter, Hardi; Tu, Chuanyi; Wang, Linghua; Zhang, Shaohua; Feng, Xueshang
刊名ASTROPHYSICAL JOURNAL
出版日期2015
卷号800期号:2页码:111
关键词magnetic reconnection Sun: corona waves
ISSN号0004-637X
通讯作者Yang, LP (reprint author), Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China.
英文摘要The Atmospheric Imaging Assembly instrument on board the Solar Dynamics Observatory has directly imaged the fast-propagating magnetosonic waves (FMWs) successively propagating outward along coronal magnetic funnels. In this study we perform a numerical investigation of the excitation of FMWs in the interchange reconnection scenario, with footpoint shearing flow being used to energize the system and drive the reconnection. The modeling results show that as a result of magnetic reconnection, the plasma in the current sheet is heated up by Joule dissipation to similar to 10 MK and is ejected rapidly, developing the hot outflows. Meanwhile, the current sheet is torn into plasmoids, which are shot quickly both upward and downward. When the plasmoids reach the outflow regions, they impact and collide with the ambient magnetic field there, which consecutively launches FMWs. The FMWs propagate outward divergently away from the impact regions, with a phase speed of the Alfven speed of similar to 1000 km s(-1). In the k-omega. diagram of the Fourier wave power, the FMWs display a broad frequency distribution with a straight ridge that represents the dispersion relation. With the WKB approximation, at the distance of 15Mm from the wave source region, we estimate the energy flux of FMWs to be E similar to 7.0 x 10(6) erg cm(-2) s(-1), which is similar to 50 times smaller than the energy flux related to the tube-channeled reconnection outflow. These simulation results indicate that energetically and dynamically the outflow is far more important than the waves.
收录类别SCI
语种英语
源URL[http://ir.nssc.ac.cn/handle/122/4648]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Yang, Liping,Zhang, Lei,He, Jiansen,et al. NUMERICAL SIMULATION OF FAST-MODE MAGNETOSONIC WAVES EXCITED BY PLASMOID EJECTIONS IN THE SOLAR CORONA[J]. ASTROPHYSICAL JOURNAL,2015,800(2):111.
APA Yang, Liping.,Zhang, Lei.,He, Jiansen.,Peter, Hardi.,Tu, Chuanyi.,...&Feng, Xueshang.(2015).NUMERICAL SIMULATION OF FAST-MODE MAGNETOSONIC WAVES EXCITED BY PLASMOID EJECTIONS IN THE SOLAR CORONA.ASTROPHYSICAL JOURNAL,800(2),111.
MLA Yang, Liping,et al."NUMERICAL SIMULATION OF FAST-MODE MAGNETOSONIC WAVES EXCITED BY PLASMOID EJECTIONS IN THE SOLAR CORONA".ASTROPHYSICAL JOURNAL 800.2(2015):111.

入库方式: OAI收割

来源:国家空间科学中心

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