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	Dynamic Jovian Magnetosphere Responses to Enhanced Solar Wind Ram Pressure: Implications for Auroral Activities 期刊论文 OAI收割 GEOPHYSICAL RESEARCH LETTERS, 2022, 卷号: 49, 期号: 19, 页码: 9 作者: Feng, Enhao; Zhang, Binzheng; Yao, Zhonghua \| 收藏 \| 浏览/下载：31/0 \| 提交时间：2023/04/03 Jovian magnetosphere Jovian aurora enhanced solar wind global MHD simulation field-aligned currents Alfvenic power
	Unusual Multiple Excitation of Large-Scale Gravity Waves by Successive Stream Interactions: The Role of Alfvenic Fluctuations 期刊论文 OAI收割 JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019, 卷号: 124, 期号: 7, 页码: 6281-6287 作者: Guo, Jianpeng; Wang, Zehao; Zheng, Jianchuan; Cui, Jun; Wei, Yong \| 收藏 \| 浏览/下载：63/0 \| 提交时间：2019/10/21 Alfvenic fluctuations gravity wave
	Unusual Multiple Excitation of Large-Scale Gravity Waves by Successive Stream Interactions: The Role of Alfvenic Fluctuations 期刊论文 OAI收割 JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019, 卷号: 124, 期号: 7, 页码: 6281-6287 作者: Guo, Jianpeng; Wang, Zehao; Zheng, Jianchuan; Cui, Jun; Wei, Yong \| 收藏 \| 浏览/下载：17/0 \| 提交时间：2020/03/10 Alfvenic fluctuations gravity wave
	Contribution of ULF Wave Activity to the Global Recovery of the Outer Radiation Belt During the Passage of a High-Speed Solar Wind Stream Observed in September 2014 期刊论文 OAI收割 JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019, 卷号: 124, 期号: 3, 页码: 1660-1678 作者: Da Silva, L. A.; Sibeck, D.; Alves, L. R.; Souza, V. M.; Jauer, P. R. \| 收藏 \| 浏览/下载：58/0 \| 提交时间：2019/07/10 radiation belts ULF wave relativistic electron flux Earth's magnetosphere high-speed stream Alfvenic fluctuations
	Measurements of the Vorticity in the Bursty Bulk Flows 期刊论文 OAI收割 GEOPHYSICAL RESEARCH LETTERS, 2019, 卷号: 46, 期号: 17-18, 页码: 10322-10329 作者: Zhang, L.Q.; Baumjohann, W.; Dai, L.; Khotyaintsev, Yu V.; Wang, C. \| 收藏 \| 浏览/下载：66/0 \| 提交时间：2019/12/17 vorticity flow eddy bursty bulk flows Curlometer analysis kinetic Alfvenic wave
	Velocity Anisotropy in Self-gravitating Molecular Clouds. I. Simulation 期刊论文 OAI收割 Astrophysical Journal, 2017, 卷号: 836, 期号: 1, 页码: 1495 作者: Otto, Frank; Ji, Weiguang; Li, Hua-bai \| 收藏 \| 浏览/下载：20/0 \| 提交时间：2019/12/09 gravitation ISM: kinematics and dynamics ISM: magnetic fields ISM: structure magnetohydrodynamics (MHD) turbulence compressible magnetohydrodynamic turbulence magnetic-field alfvenic turbulence interstellar-medium dissipation statistics Astronomy & Astrophysics
	Solitary kinetic Alfven waves in dusty plasmas 期刊论文 OAI收割 PHYSICS OF PLASMAS, 2008, 卷号: 15, 期号: 8, 页码: 083703 作者: Li, Yang-fang; Wu, D. J.; Morfill, G. E. 收藏 \| 浏览/下载：33/0 \| 提交时间：2011/12/29 Solitary kinetic Alfven waves in dusty plasmas are studied by Considering the dust charge variation. The effect of the dust charge-to-mass ratio on the soliton solution is discussed. The Sagdeev potential is derived analytically with constant dust charge and then calculated numerically by taking the dust charge variation into account. We show that the dust charge-to-mass ratio plays an important role in the soliton properties. The soliton solutions are comprised of two branches. One branch is sub-Alfvenic and the soliton velocity is obviously smaller than the Alfven speed. The other branch is super-Alfvenic and the soliton velocity is very close to or greater than the Alfven speed. Both compressive and rarefactive solitons can exist. For the sub-Alfvenic branch the rarefactive soliton is bell-shaped and it is much narrower than the compressive one. However for the super-Alfvenic branch the compressive soliton is bell-shaped and narrower and the rarefactive one is broadened. When the charge-to-mass ratio of the dust grains is sufficiently high the width of the rarefactive soliton in the super-Alfvenic branch will broaden extremely and a electron depletion will be observed. It is also shown that the bell-shaped soliton can transition to a cusped structure when the velocity is sufficiently high. (C) 2008 American Institute of Physics.