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
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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 |
DOI | 10.3847/2041-8213/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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