Statistical Properties of Small-scale Linear Magnetic Holes in the Martian Magnetosheath
文献类型:期刊论文
作者 | Wu, Mingyu2,3; Chen, Yangjun2; Du, Aimin4; Wang, Guoqiang2; Xiao, Sudong2; Peng, E.6; Pan, Zonghao1; Chen, Yuanqiang1; Zhang, Tielong2,5 |
刊名 | ASTROPHYSICAL JOURNAL
![]() |
出版日期 | 2021-08-01 |
卷号 | 916期号:2页码:7 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ac090b |
英文摘要 | The small-scale linear magnetic hole (LMH) is a magnetic dip with a size less than or on the order of rho ( i ) (proton gyroradius), which may contribute to turbulence properties in the solar wind and other astrophysical plasmas. Based on one-month measurements of the Mars Atmosphere and Volatile EvolutioN mission, 174 small-scale LMH events in the Martian magnetosheath are used to investigate their statistical properties in this study. Our results show that small-scale linear LMHs are ubiquitous in the Martian magnetosheath, and their occurrence rate is estimated to be approximately 1.5 events per hour based on one-month observations. Compared with the ambient plasma, the averaged magnitude of the magnetic field in these holes can decrease from 6.8-3.5 nT. Nearly 66% of events have a B (min)/B value in the range of (0.45, 0.75). The duration of small-scale MHs is mainly less than 0.4 s. For 90% of the events, the size along the solar wind flow is less than rho ( i ). As the rotation angle increases, the occurrence rate of small-scale LMHs decrease. However, the B (min)/B, size, and duration of small-scale LMHs have no obvious dependence on their rotation angle. |
WOS关键词 | MIRROR INSTABILITY ; SOLAR-WIND ; DYNAMICS ; WAVES |
资助项目 | NSFC[41774167] ; NSFC[41774171] ; NSFC[41974205] ; NSFC[41804157] ; NSFC[11975086] ; NSFC[41904156] ; preresearch Project on Civil Aerospace Technologies - CNSA[D020103] ; Shenzhen Science and Technology Program[KQTD20180410161218820] ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; CAS Center for Excellence in Comparative Planetology |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000681056300001 |
出版者 | IOP PUBLISHING LTD |
资助机构 | NSFC ; NSFC ; preresearch Project on Civil Aerospace Technologies - CNSA ; preresearch Project on Civil Aerospace Technologies - CNSA ; Shenzhen Science and Technology Program ; Shenzhen Science and Technology Program ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; CAS Center for Excellence in Comparative Planetology ; CAS Center for Excellence in Comparative Planetology ; NSFC ; NSFC ; preresearch Project on Civil Aerospace Technologies - CNSA ; preresearch Project on Civil Aerospace Technologies - CNSA ; Shenzhen Science and Technology Program ; Shenzhen Science and Technology Program ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; CAS Center for Excellence in Comparative Planetology ; CAS Center for Excellence in Comparative Planetology ; NSFC ; NSFC ; preresearch Project on Civil Aerospace Technologies - CNSA ; preresearch Project on Civil Aerospace Technologies - CNSA ; Shenzhen Science and Technology Program ; Shenzhen Science and Technology Program ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; CAS Center for Excellence in Comparative Planetology ; CAS Center for Excellence in Comparative Planetology ; NSFC ; NSFC ; preresearch Project on Civil Aerospace Technologies - CNSA ; preresearch Project on Civil Aerospace Technologies - CNSA ; Shenzhen Science and Technology Program ; Shenzhen Science and Technology Program ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; Key Laboratory of Lunar and Deep Space Exploration, CAS ; CAS Center for Excellence in Comparative Planetology ; CAS Center for Excellence in Comparative Planetology |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/101913] ![]() |
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 | Wu, Mingyu; Zhang, Tielong |
作者单位 | 1.Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei 230026, Peoples R China 2.Harbin Inst Technol, Inst Space Sci & Appl Technol, Shenzhen, Peoples R China 3.Chinese Acad Sci, Key Lab Lunar & Deep Space Explorat, Beijing, Peoples R China 4.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China 5.Austrian Acad Sci, Space Res Inst, Graz, Austria 6.Harbin Inst Technol, Lab Space Environm & Phys Sci, Harbin, Peoples R China |
推荐引用方式 GB/T 7714 | Wu, Mingyu,Chen, Yangjun,Du, Aimin,et al. Statistical Properties of Small-scale Linear Magnetic Holes in the Martian Magnetosheath[J]. ASTROPHYSICAL JOURNAL,2021,916(2):7. |
APA | Wu, Mingyu.,Chen, Yangjun.,Du, Aimin.,Wang, Guoqiang.,Xiao, Sudong.,...&Zhang, Tielong.(2021).Statistical Properties of Small-scale Linear Magnetic Holes in the Martian Magnetosheath.ASTROPHYSICAL JOURNAL,916(2),7. |
MLA | Wu, Mingyu,et al."Statistical Properties of Small-scale Linear Magnetic Holes in the Martian Magnetosheath".ASTROPHYSICAL JOURNAL 916.2(2021):7. |
入库方式: OAI收割
来源:地质与地球物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。