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Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST
Li, Dong; Shen, Yuandeng; Ning, Zongjun; Zhang, Qingmin; Zhou, Tuanhui; Li, D (reprint author), Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China.; Li, D (reprint author), Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R China.; Li, D (reprint author), Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100012, Peoples R China.
Department微波遥感部
Source PublicationASTROPHYSICAL JOURNAL
2018
Volume863Issue:2Pages:192
ISSN0004-637X
Language英语
KeywordInstabilities Magnetohydrodynamics (Mhd) Sun: Chromosphere Sun: Oscillations Sun: Filaments Prominences
AbstractWe present high-resolution observations of two kinds of dynamic behavior in a quiescent prominence using the New Vacuum Solar Telescope, i.e., Kelvin-Helmholtz instabilities (KHIs) and small-scale oscillations. The KHIs were identified as rapidly developed vortex-like structures with counterclockwise/clockwise rotations in the Ha red-wing images at +0.3 angstrom, which were produced by the strong shear-flow motions on the surface/interface of prominence plumes. The KHI growth rates are estimated to be similar to 0.0135 +/- 0.0004 and similar to 0.0138 +/- 0.0004. Our observational results further suggest that the shear velocities (i.e., supersonic) of the mass flows are fast enough to produce the strong deformation of the boundary and overcome the restraining surface tension force. This flowdriven instability might play a significant role in the process of plasma transfer in solar prominences. The smallscale oscillations perpendicular to the prominence threads are observed in the Ha line-center images. The oscillatory periods changed nonmonotonically and showed two changing patterns, in which one first decreased slowly and then started to increase, while the other grew fast at the beginning and then started to decrease. Both of these thread oscillations with changing periods were observed to be unstable for an entire cycle, and they were local in nature. All our findings indicate that the small-scale thread oscillations could be magnetohydrodynamic waves in the solar corona.
Indexed BySCI
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/6436
Collection微波遥感部
Corresponding AuthorLi, D (reprint author), Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China.; Li, D (reprint author), Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R China.; Li, D (reprint author), Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100012, Peoples R China.
Recommended Citation
GB/T 7714
Li, Dong,Shen, Yuandeng,Ning, Zongjun,et al. Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST[J]. ASTROPHYSICAL JOURNAL,2018,863(2):192.
APA Li, Dong.,Shen, Yuandeng.,Ning, Zongjun.,Zhang, Qingmin.,Zhou, Tuanhui.,...&Li, D .(2018).Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST.ASTROPHYSICAL JOURNAL,863(2),192.
MLA Li, Dong,et al."Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST".ASTROPHYSICAL JOURNAL 863.2(2018):192.
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20188632192.pdf(1907KB)期刊论文作者接受稿开放获取CC BY-NC-SAApplication Full Text
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