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DOI | 10.1029/2020GL087559 |
Nonlinear Response of the Cross Polar Cap Potential to Solar Wind Density Under Northward Interplanetary Magnetic Field | |
Yang Z.; Zhang B.; Lei J.; Dang T. | |
发表日期 | 2020 |
ISSN | 0094-8276 |
卷号 | 47期号:8 |
英文摘要 | It is commonly believed that the magnitude and orientation of interplanetary magnetic field (IMF) together with the solar wind (SW) velocity have the most important impact on the cross polar cap potential (φpc), so that little attention has been given to the effect of SW density, especially under northward IMF conditions. Previous studies have shown that φpc increases with SW density as a response to the changes in magnetosheath force balance, while our study shows that φpc has more complicated responses to the SW density depending on the magnitude of IMF rather than a simple linear response as reported previously. The φpc may be insensitive to SW density increasing at moderate IMF Bz (cf. 8 nT) and at intense Bz (20 nT) under large-density conditions. The different behavior of SW density in regulating φpc is mainly due to the competing effects originated from viscous interaction and magnetic reconnection. Further, the physical mechanisms are explored, including the driving sources of the viscous potential and affecting factors of reconnection potential. These results pave the way for better understanding of the SW density effects on solar wind-magnetosphere-ionosphere (SW-M-I) interactions. ©2020. American Geophysical Union. All Rights Reserved. |
英文关键词 | Ionosphere; Magnetic fields; Magnetosphere; Competing effects; Cross polar cap potential; Interplanetary magnetic fields; Magnetic reconnections; Non-linear response; Physical mechanism; Solar wind density; Viscous interaction; Solar wind; ionosphere; magnetic field; magnetosphere; solar wind |
语种 | 英语 |
来源期刊 | Geophysical Research Letters
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/170435 |
作者单位 | CAS Key Laboratory of Geospace Environment, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China; CAS Center for Excellence in Comparative Planetology, University of Science and Technology of China, Hefei, China; Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China; Department of Earth Sciences, The University of Hong Kong, Pokfulam, China |
推荐引用方式 GB/T 7714 | Yang Z.,Zhang B.,Lei J.,et al. Nonlinear Response of the Cross Polar Cap Potential to Solar Wind Density Under Northward Interplanetary Magnetic Field[J],2020,47(8). |
APA | Yang Z.,Zhang B.,Lei J.,&Dang T..(2020).Nonlinear Response of the Cross Polar Cap Potential to Solar Wind Density Under Northward Interplanetary Magnetic Field.Geophysical Research Letters,47(8). |
MLA | Yang Z.,et al."Nonlinear Response of the Cross Polar Cap Potential to Solar Wind Density Under Northward Interplanetary Magnetic Field".Geophysical Research Letters 47.8(2020). |
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