中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Propagation properties of foreshock cavitons: Cluster observations

文献类型:期刊论文

作者Wang, MengMeng1,2; Yao, ShuTao1; Shi, QuanQi1; Zhang, Hui3; Tian, AnMin1; Degeling, Alexander William1; Zhang, Shuai1; Guo, RuiLong4; Sun, WeiJie5; Liu, Ji2
刊名SCIENCE CHINA-TECHNOLOGICAL SCIENCES
出版日期2020
卷号63期号:1页码:173-182
关键词foreshock transient phenomena cavitons nonlinear evolution of ULF waves propagation and evolution properties of structures multipoint spacecraft methods
ISSN号1674-7321
DOI10.1007/s11431-018-9450-3
英文摘要Foreshock cavitons are transient phenomena observed in the terrestrial foreshock region. They are characterized by a simultaneous depression of magnetic field magnitude and plasma density, which are bounded with enhancements of these two parameters and surrounded by ultralow frequency (ULF) waves. Previous studies focused on the interplanetary magnetic field (IMF) conditions, solar wind (SW) conditions, and the growth of the foreshock waves related to the generation of foreshock cavitons. Previously, a multipoint spacecraft analysis method using Cluster data was applied to analyze only two foreshock cavitons, and this method did not consider uncertainties. In this study, multipoint spacecraft analysis methods, including the timing method, the minimum directional derivative (MDD) method, and the spatiotemporal difference (STD) method are applied to determine the velocity in both spacecraft and solar wind frames. The propagation properties show good agreement with previous results from simulations and observations that most cavitons move sunward in the solar wind frame, with the velocities larger than the Alfven speed. The propagation properties of foreshock cavitons support the formation mechanism of cavitons in previous simulations, which suggested that cavitons are formed due to the nonlinear evolution of compressive ULF waves. We find that there is clear decreasing trend between the size of cavitons and their velocity in the solar wind frame. In addition, the timing method considering errors has been applied to study the evolution properties by comparing the velocities with errors of the leading and trailing edges, and we identify three stable cavitons and one contracting caviton, which has not been studied before. Most cavitons should remain stable when they travel toward the Earth's bow shock. The relationship between the size of foreshock cavitons and their distance from the bow shock is also discussed.
WOS关键词HOT FLOW ANOMALIES ; MAGNETIC HOLES ; SOLAR-WIND ; BOW SHOCK ; ULF WAVES ; GENERATION ; CAVITIES ; EVENTS
WOS研究方向Engineering ; Materials Science
语种英语
WOS记录号WOS:000511855100016
出版者SCIENCE PRESS
源URL[http://ir.iggcas.ac.cn/handle/132A11/95691]  
专题地质与地球物理研究所_中国科学院地球与行星物理重点实验室
通讯作者Shi, QuanQi
作者单位1.Shandong Univ, Sch Space Sci & Phys, Weihai 264209, Peoples R China
2.Chinese Acad Sci, Natl Space Sci Ctr, Beijing 100190, Peoples R China
3.Univ Alaska Fairbanks, Inst Geophys, Fairbanks, AK 99775 USA
4.Chinese Acad Sci, Inst Geol & Geophys, Beijing 100029, Peoples R China
5.Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48113 USA
6.Peking Univ, Inst Space Phys & Appl Technol, Beijing 100871, Peoples R China
推荐引用方式
GB/T 7714
Wang, MengMeng,Yao, ShuTao,Shi, QuanQi,et al. Propagation properties of foreshock cavitons: Cluster observations[J]. SCIENCE CHINA-TECHNOLOGICAL SCIENCES,2020,63(1):173-182.
APA Wang, MengMeng.,Yao, ShuTao.,Shi, QuanQi.,Zhang, Hui.,Tian, AnMin.,...&Pu, ZuYin.(2020).Propagation properties of foreshock cavitons: Cluster observations.SCIENCE CHINA-TECHNOLOGICAL SCIENCES,63(1),173-182.
MLA Wang, MengMeng,et al."Propagation properties of foreshock cavitons: Cluster observations".SCIENCE CHINA-TECHNOLOGICAL SCIENCES 63.1(2020):173-182.

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来源:地质与地球物理研究所

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