Magnetic cloud observations from MESSENGER and Venus Express

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户:good240
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
We present statistical findings from a recently compiled catalogue of magnetic clouds observed by the MESSENGER and Venus Express spacecraft. Despite their planetary focus, both spacecraft spent significant amounts of time in the solar wind, allowing transient solar wind structures such as magnetic clouds to be observed.
其他文献
Previous studies of magnetic reconnection in the solar wind have suggested that a single reconnection X-line can extend and be active over millions of kilometres.
会议
Zank et al.2012 developed a turbulence transport model for low-frequency incompressible magnetohydrodynamic(MHD) turbulence in inhomogeneous flows in terms of the energy corresponding to the forward a
会议
The parametric instabilities of an Alfven wave in a proton-electron plasma system are found to have great influence on proton dynamics,where part of the protons can be accelerated through the Landau r
会议
In solar wind,magnetohydrodynamic(MHD) discontinuities are ubiquitous and often found to be at the origin of turbulence intermittency.They may also play a key role in the turbulence dissipation and he
会议
Both coronal mass ejections(CMEs) and corotating interaction regions(CIRs) can be sources of space weather disaster.The impact of fast shock on magnetic cloud is a pivotal process in CME-CME interacti
会议
During the quiet time when the interplanetary magnetic field(IMF) is northward,using Cluster multi-spacecraftdata between August and October from 2002 to 2004,Shi et al.
会议
Prediction of the shocks arrival times(SATs) at the Earth is very important for space weather forecast.There is a well-known SAT model,STOA,which is widely used in the space weather forecast.
会议
The solar coronal field forms an important link between the underlying source in the solar photosphere and the heliospheric magnetic field emanating away from the Sun with the solar wind.Since the cor
会议
We investigate properties of the plasma fluid motion in the large amplitude low frequency fluctuations of highly Alfvénic fast solar wind.We show that protons locally conserve total kinetic energy whe
会议
Intermittency is a significant component of solar wind turbulence,and appears to be closely connected with the spectral anisotropy of turbulence.We use the Local Intermittency Measure(LIM) to identify
会议