Effects of Orbital Eccentricity and IMF Cone Angle on the Dimensions of Mercury's Magnetosphere
文献类型:期刊论文
作者 | Zhong, J.3; Shue, J. -H.2; Wei, Y.3; Slavin, J. A.1; Zhang, H.3; Rong, Z. J.3; Chai, L. H.3; Wan, W. X.3 |
刊名 | ASTROPHYSICAL JOURNAL
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出版日期 | 2020-03-20 |
卷号 | 892期号:1页码:7 |
关键词 | Planetary magnetosphere Solar-planetary interactions Mercury (planet) Solar wind Interplanetary magnetic fields Solar magnetic reconnection |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ab7819 |
英文摘要 | We investigate the influence of orbital eccentricity and interplanetary magnetic field (IMF) direction on the dimensions of Mercury's magnetosphere using four Earth years of data collected by the MErcury Surface, Space ENvironment, GEochemistry, and Ranging spacecraft. The variations in magnetopause subsolar distance, flank distance, and tail radius are compared to determine the global dimensions and compressibility of the magnetosphere. As Mercury moves from perihelion (aphelion) to aphelion (perihelion) its magnetosphere expands (contracts) globally by similar to 15% on average. After mapping all of the magnetopause crossings to a fixed radial distance from the Sun, we find that IMF cone angle changes lead to reconfigurations of the magnetosphere of comparable magnitude to radial solar distance effects. Furthermore, the magnetosphere is found to expand globally under the quasi-radial IMF, while contracting under the quasi-perpendicular conditions. A new Mercury magnetopause model parameterized by the heliocentric distance and IMF cone angle was constructed. Unlike Earth, the model gives a closed magnetopause for the nightside in most cases, and its flaring decreases with the contraction of the magnetosphere. The results demonstrate the highly variable reconfigurations of Mercury's magnetosphere under its extreme environmental conditions. |
WOS关键词 | MAGNETIC-FLUX TRANSFER ; MESSENGER OBSERVATIONS ; SOLAR-WIND ; BOW SHOCK ; DAYSIDE MAGNETOSPHERE ; MAGNETOPAUSE ; FIELD ; SURFACE ; EVENTS ; INSTRUMENT |
资助项目 | Strategic Priority Research Program of the Chinese Academy of Sciences[XDA17010201] ; National Natural Science Foundation of China[41674178] ; National Natural Science Foundation of China[41874198] ; National Natural Science Foundation of China[41621004] ; NASA Discovery Data Analysis Grant[80NSSC18K1137] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000521413500001 |
出版者 | IOP PUBLISHING LTD |
资助机构 | Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NASA Discovery Data Analysis Grant ; NASA Discovery Data Analysis Grant ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NASA Discovery Data Analysis Grant ; NASA Discovery Data Analysis Grant ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NASA Discovery Data Analysis Grant ; NASA Discovery Data Analysis Grant ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NASA Discovery Data Analysis Grant ; NASA Discovery Data Analysis Grant |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/94058] ![]() |
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 | Zhong, J. |
作者单位 | 1.Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA 2.Natl Cent Univ, Inst Space Sci, Taoyuan, Taiwan 3.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Zhong, J.,Shue, J. -H.,Wei, Y.,et al. Effects of Orbital Eccentricity and IMF Cone Angle on the Dimensions of Mercury's Magnetosphere[J]. ASTROPHYSICAL JOURNAL,2020,892(1):7. |
APA | Zhong, J..,Shue, J. -H..,Wei, Y..,Slavin, J. A..,Zhang, H..,...&Wan, W. X..(2020).Effects of Orbital Eccentricity and IMF Cone Angle on the Dimensions of Mercury's Magnetosphere.ASTROPHYSICAL JOURNAL,892(1),7. |
MLA | Zhong, J.,et al."Effects of Orbital Eccentricity and IMF Cone Angle on the Dimensions of Mercury's Magnetosphere".ASTROPHYSICAL JOURNAL 892.1(2020):7. |
入库方式: OAI收割
来源:地质与地球物理研究所
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