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[期刊论文] 作者:Eckart Marsch, 来源:现代物理(英文) 年份:2015
A real version of the Dirac equation is derived and its coupling to the electromagnetic field considered. First the four-component real Majorana equation is bri...
[期刊论文] 作者:Eckart Marsch, 来源:现代物理(英文) 年份:2011
We revisit the two-component Majorana equation and derive it in a new form by linearizing the relativistic dispersion relation of a massive particle, in a way s...
[会议论文] 作者:Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
The solar wind is permeated by all kinds of fluctuations ranging broadly inscales from those of the solar corona and inner heliosphere down to the local ionand electron plasma kinetic scales....
[期刊论文] 作者:覃争锐, 涂传诒, Eckart Marsch, 来源:空间科学学报 年份:2004
利用Helios2飞船的数据,对太阳风速度分布中质子束流部分与整个质子的密度之比随日心距离的变化做了分析.为了排除碰撞因素的影响,有针对性地分析了太阳风高速流(600<vs<700km/...
[会议论文] 作者:Linghua Wang,Jiansen He,Chuanyi Tu,Xin Wang,Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Linghua Wang,Jiansen He,Xin Wang,Chuanyi Tu,Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Chuanyi Tu,Jiansen He,Xin Wang,Linghua Wang,Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Xin Wang,Chuanyi Tu,Jiansen He,Eckart Marsch,Linghua Wang, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
Two different explanations have been suggested for the recent finding on the anisotropy of the solar wind turbulence power spectrum at the high-frequency end of the inertial range:1.a "critical balanc...
[会议论文] 作者:Xin Wang,Chuanyi Tu,Jiansen He,Eckart Marsch,Linghua Wang, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
It was recently reported that the spectral slope and the correlation function of the magnetic field in the solar wind turbulence are anisotropic when they are based on continuous time series with loca...
[会议论文] 作者:Chuanyi Tu,Xin Wang,Jiansen He,Eckart Marsch,Linghua Wang, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
The slow solar wind turbulence has recently been considered as fully evolved turbulence which can be described by GS theory.However,here we present new findings that support a different understanding....
[会议论文] 作者:姚硕,何健森,涂传诒,王玲华,Eckart Marsch, 来源:2015年中国地球科学联合学术年会 年份:2015
[会议论文] 作者:姚硕,何建森,涂传诒,王玲华,Eckart Marsch, 来源:2014年中国地球科学联合学术年会 年份:2014
本工作探究当局地磁场矢量与太阳风速度矢量反平行和近垂直时的小尺度压力平衡结构的成因。通过分析WIND 卫星在1AU 处测量的平静太阳风中的等离子体和磁场数据,并引入磁流体力学波模的理论计算参数与实测数据比对,从而判别波模。更关键地,探究了太阳风中的质子分......
[会议论文] 作者:Linghua Wang,Zhongtian Pei,Limei Yan,Chuanyi Tu,Xin Wang,Jiansen He,Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Linghua Wang,Chuanyi Tu,Wenzhi Ruan,Lei Zhang,Jiansen He,Christian Vocks,Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Chuanyi Tu,Linghua Wang,Jiansen He,Xin Wang,Lei Zhang,Zhongtian Pei,Eckart Marsch, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:裴仲添,何建森,涂传诒,Eckart Marsch,王玲华, 来源:2016中国地球科学联合学术年会 年份:2016
在太阳风湍流中,耗散区间歇的特性越来越多的受到人们关注.在本工作中,研究磁场扰动的平整度(即峰度),并按照不同的时间尺度和局地背景磁场与日地径向方向的夹角来计算平整度的分布.这一分布呈现出蝴蝶图样式的特征,两翼位于平行/反平行方向上.蝴蝶图意味着在平......
[会议论文] 作者:Lei Zhang,Li-Ping Yang,Jian-Sen He,Chuan-Yi Tu,Ling-hua Wang,Eckart Marsch,Xue-Shang Feng, 来源:2014年中国地球科学联合学术年会 年份:2014
In solar wind,slow mode magnetosonic waves are scarce to be identified,but their dissipation plays one of key roles in heating the solar wind,and the wave mode contributes essentially to the solar win...
[会议论文] 作者:Zhongtian Pei,Jiansen He,Xin Wang,Chuanyi Tu,Eckart Marsch,Linghua Wang,Limei Yan, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
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...
[会议论文] 作者:Jiansen He,Chuanyi Tu,Eckart Marsch,Linghua Wang,Zhongtian Pei,Lei Zhang,Xin Wang, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
The Solar wind is observed to expand outward non-adiabatically.The energy source for the non-adiabatic behavior is commonly attributed to the solar wind turbulence....
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