中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
On the ionospheric source region of cold ion outflow

文献类型:期刊论文

作者Li, K.; Haaland, S.; Eriksson, A.; Andre, M.; Engwall, E.; Wei, Y.; Kronberg, E. A.; Fraenz, M.; Daly, P. W.; Zhao, H.
刊名GEOPHYSICAL RESEARCH LETTERS
出版日期2012
卷号39页码:L18102
ISSN号0094-8276
通讯作者Haaland, S (reprint author), Max Planck Inst Solar Syst Res, Max Planck Str 2, DE-37191 Katlenburg Lindau, Germany.
中文摘要Recent studies have shown that low energy ions constitute a significant part of the total ion population in the Earth's magnetosphere. In this study, we have used a comprehensive data set with measurements of cold (total energy less than 70 eV) ion velocity and density to determine their source. This data set is derived from Cluster satellite measurements combined with solar wind and interplanetary magnetic field measurements and geomagnetic indices. By using the guiding center equation of motion, we were able to calculate the trajectories and thus determine the source region of the cold ions. Our results show that the polar cap region is the primary source for cold ions. We also found that the expansion and contraction of the polar cap as a consequence of changes in solar wind parameters were correlated with the source region size and intensity of the cold ion outflow. Elevated outflow fluxes near the nightside auroral zone and the dayside cusps during disturbed conditions suggest that energy and particle precipitation from the magnetosphere or directly from the solar wind can enhance the outflow of cold ions from the ionosphere. Citation: Li, K., et al. (2012), On the ionospheric source region of cold ion outflow, Geophys. Res. Lett., 39, L18102, doi:10.1029/2012GL053297.
英文摘要Recent studies have shown that low energy ions constitute a significant part of the total ion population in the Earth's magnetosphere. In this study, we have used a comprehensive data set with measurements of cold (total energy less than 70 eV) ion velocity and density to determine their source. This data set is derived from Cluster satellite measurements combined with solar wind and interplanetary magnetic field measurements and geomagnetic indices. By using the guiding center equation of motion, we were able to calculate the trajectories and thus determine the source region of the cold ions. Our results show that the polar cap region is the primary source for cold ions. We also found that the expansion and contraction of the polar cap as a consequence of changes in solar wind parameters were correlated with the source region size and intensity of the cold ion outflow. Elevated outflow fluxes near the nightside auroral zone and the dayside cusps during disturbed conditions suggest that energy and particle precipitation from the magnetosphere or directly from the solar wind can enhance the outflow of cold ions from the ionosphere. Citation: Li, K., et al. (2012), On the ionospheric source region of cold ion outflow, Geophys. Res. Lett., 39, L18102, doi:10.1029/2012GL053297.
学科主题空间物理
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/122/3225]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Li, K.,Haaland, S.,Eriksson, A.,et al. On the ionospheric source region of cold ion outflow[J]. GEOPHYSICAL RESEARCH LETTERS,2012,39:L18102.
APA Li, K..,Haaland, S..,Eriksson, A..,Andre, M..,Engwall, E..,...&Ren, Q. Y..(2012).On the ionospheric source region of cold ion outflow.GEOPHYSICAL RESEARCH LETTERS,39,L18102.
MLA Li, K.,et al."On the ionospheric source region of cold ion outflow".GEOPHYSICAL RESEARCH LETTERS 39(2012):L18102.

入库方式: OAI收割

来源:国家空间科学中心

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