中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Observational Evidence for Fast Mode Periodic Small-scale Shocks: A New Type of Plasma Phenomenon

文献类型:期刊论文

作者Shan, Lican2,3; Tsurutani, Bruce T.4; Ohsawa, Yukiharu5; Mazelle, Christian6; Huang, Can2,3; Du, Aimin2,3,7,9; Ge, Yasong S.2,3,9; Lu, Quanming1,8
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2020-12-01
卷号905期号:1页码:6
关键词Interplanetary shocks Planetary bow shocks Solar coronal mass ejection shocks Stellar bow shocks
ISSN号2041-8205
DOI10.3847/2041-8213/abcb02
英文摘要We show observational evidence for a new form of collisionless shock in interplanetary space near Mars, small-scale shocks with periodic spacings. Pickup of new ionized hydrogen atoms in a magnetic field aligned with the solar wind direction causes the generation of a magnetosonic wave train through an ion beam instability. The waves have a frequency close to the local proton gyrofrequency. This is a similar physical process as for the formation of cometary plasma waves/turbulence. However, for the case of proton pickup near Mars, each individual magnetosonic wave cycle develops into a small-scale shock. So there is a string of fast mode shocks formed with proton gyroperiod spacings. These small-scale shocks display dissipation in the ions and dispersive whistlers. A fraction of ions trapped/reflected at the small-scale shocks are accelerated by the motional electric field. Observational results demonstrate that periodic shocks can perform the same functions as a single supercritical shock in a high-speed flow.
WOS关键词SOLAR-WIND INTERACTION ; GRIGG-SKJELLERUP ; BOW SHOCK ; IONS ; WAVES ; INSTABILITIES ; FREQUENCY ; ACCELERATION ; TURBULENCE ; UPSTREAM
资助项目National Natural Science Foundation of China[41774187] ; National Natural Science Foundation of China[41974173] ; National Natural Science Foundation of China[41874080] ; National Natural Science Foundation of China[41674168] ; National Natural Science Foundation of China[41874197] ; Beijing Municipal Science and Technology Commission[Z191100004319001] ; Strategic Priority Research Program of Chinese Academy of Sciences[XDB41010304] ; pre-research Project on Civil Aerospace Technologies - CNSA[D020103] ; NASA
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000596720200001
出版者IOP PUBLISHING LTD
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; Beijing Municipal Science and Technology Commission ; Beijing Municipal Science and Technology Commission ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; pre-research Project on Civil Aerospace Technologies - CNSA ; pre-research Project on Civil Aerospace Technologies - CNSA ; NASA ; NASA ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Beijing Municipal Science and Technology Commission ; Beijing Municipal Science and Technology Commission ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; pre-research Project on Civil Aerospace Technologies - CNSA ; pre-research Project on Civil Aerospace Technologies - CNSA ; NASA ; NASA ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Beijing Municipal Science and Technology Commission ; Beijing Municipal Science and Technology Commission ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; pre-research Project on Civil Aerospace Technologies - CNSA ; pre-research Project on Civil Aerospace Technologies - CNSA ; NASA ; NASA ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Beijing Municipal Science and Technology Commission ; Beijing Municipal Science and Technology Commission ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; pre-research Project on Civil Aerospace Technologies - CNSA ; pre-research Project on Civil Aerospace Technologies - CNSA ; NASA ; NASA
源URL[http://ir.iggcas.ac.cn/handle/132A11/98774]  
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Shan, Lican
作者单位1.Univ Sci & Technol China, CAS Key Lab Geospace Environm, Hefei 230026, Peoples R China
2.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
3.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing 100029, Peoples R China
4.CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
5.Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
6.Univ Paul Sabatier, CNRS, Inst Rech Astrophys & Planetol, F-31400 Toulouse, France
7.Macau Univ Sci & Technol, Macau 999078, Peoples R China
8.CAS Ctr Excellence Comparat Planetol, Hefei 230026, Peoples R China
9.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing 100049, Peoples R China
推荐引用方式
GB/T 7714
Shan, Lican,Tsurutani, Bruce T.,Ohsawa, Yukiharu,et al. Observational Evidence for Fast Mode Periodic Small-scale Shocks: A New Type of Plasma Phenomenon[J]. ASTROPHYSICAL JOURNAL LETTERS,2020,905(1):6.
APA Shan, Lican.,Tsurutani, Bruce T..,Ohsawa, Yukiharu.,Mazelle, Christian.,Huang, Can.,...&Lu, Quanming.(2020).Observational Evidence for Fast Mode Periodic Small-scale Shocks: A New Type of Plasma Phenomenon.ASTROPHYSICAL JOURNAL LETTERS,905(1),6.
MLA Shan, Lican,et al."Observational Evidence for Fast Mode Periodic Small-scale Shocks: A New Type of Plasma Phenomenon".ASTROPHYSICAL JOURNAL LETTERS 905.1(2020):6.

入库方式: OAI收割

来源:地质与地球物理研究所

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