中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Outward expansion of the lunar wake: ARTEMIS observations

文献类型:期刊论文

作者Zhang, H.; Khurana, K. K.; Zong, Q. -G.; Kivelson, M. G.; Hsu, T. -S.; Wan, W. X.; Pu, Z. Y.; Angelopoulos, V.; Cao, X.; Wang, Y. F.
刊名GEOPHYSICAL RESEARCH LETTERS
出版日期2012
卷号39页码:L18104
ISSN号0094-8276
通讯作者Zhang, H (reprint author), Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China.
中文摘要Magnetohydrodynamics (MHD) predicts that lunar wake expands outward at magnetosonic velocities in all directions perpendicular to background solar wind; however, fluid theories emphasize that lunar wake expands outward at sound speeds mainly along the interplanetary magnetic field (IMF). Early observations supported the MHD predictions in the near-moon region despite lack of solar wind and IMF observations. Thanks to the special orbit design of the ARTEMIS mission, the solar wind conditions are well determined at the time of concurrent observations in the lunar wake. 164 wake crossings made by ARTEMIS are statistically studied in this paper. Observations indicated that, in either distant or near-Moon regions, the lunar wake expands outward at the fast MHD wave velocities. This simple model provides a powerful way to determine wake boundaries, particularly at large distances where the boundary signatures are indistinct, thus allowing further studies on the Moon-solar wind/crustal field-solar wind interactions. Citation: Zhang, H., et al. (2012), Outward expansion of the lunar wake: ARTEMIS observations, Geophys. Res. Lett., 39, L18104, doi: 10.1029/2012GL052839.
英文摘要Magnetohydrodynamics (MHD) predicts that lunar wake expands outward at magnetosonic velocities in all directions perpendicular to background solar wind; however, fluid theories emphasize that lunar wake expands outward at sound speeds mainly along the interplanetary magnetic field (IMF). Early observations supported the MHD predictions in the near-moon region despite lack of solar wind and IMF observations. Thanks to the special orbit design of the ARTEMIS mission, the solar wind conditions are well determined at the time of concurrent observations in the lunar wake. 164 wake crossings made by ARTEMIS are statistically studied in this paper. Observations indicated that, in either distant or near-Moon regions, the lunar wake expands outward at the fast MHD wave velocities. This simple model provides a powerful way to determine wake boundaries, particularly at large distances where the boundary signatures are indistinct, thus allowing further studies on the Moon-solar wind/crustal field-solar wind interactions. Citation: Zhang, H., et al. (2012), Outward expansion of the lunar wake: ARTEMIS observations, Geophys. Res. Lett., 39, L18104, doi: 10.1029/2012GL052839.
学科主题空间物理
资助信息specialized research fund for Chinese state key laboratories [Y22612A33S]; KIP Pilot Project of CAS [kzcx2-yw-123]; National Science Foundation of China [40974090, 40636032]; National Important Basic Research Project [2006CB806306, 2011CB811405]; NASA through THEMIS [443869-TM-22620]; NASA through THEMIS/ARTEMIS [NAS5-02099]; German Ministry for Economy and Technology; German Center for Aviation and Space (DLR) [50 OC 0302]
收录类别SCI ; EI
语种英语
公开日期2014-12-15
源URL[http://ir.nssc.ac.cn/handle/122/3091]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Zhang, H.,Khurana, K. K.,Zong, Q. -G.,et al. Outward expansion of the lunar wake: ARTEMIS observations[J]. GEOPHYSICAL RESEARCH LETTERS,2012,39:L18104.
APA Zhang, H..,Khurana, K. K..,Zong, Q. -G..,Kivelson, M. G..,Hsu, T. -S..,...&Tang, C. L..(2012).Outward expansion of the lunar wake: ARTEMIS observations.GEOPHYSICAL RESEARCH LETTERS,39,L18104.
MLA Zhang, H.,et al."Outward expansion of the lunar wake: ARTEMIS observations".GEOPHYSICAL RESEARCH LETTERS 39(2012):L18104.

入库方式: OAI收割

来源:国家空间科学中心

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