太阳风

然后，我们研究了太阳风湍流在离子尺度的特征，统计结果表明湍流在波矢空间是强各向异性的，Alfven-whistler波模在太阳风湍流中占主导作用。

Secondly , we make statistical study solar wind turbulence at ion scale . The results prove that the turbulence is strongly anisotropic in wave vector space within universal solar wind condition . The Alfven-whistler wave mode is dominant in the solar wind turbulence .

1997年1月事件行星际扰动在三维背景太阳风中传播的数值模拟

Numerical simulation for propagation of interplanetary disturbance in three dimensional solar wind background during January 1997 event

太阳风在日冕磁漏斗状结构中的起源&介绍一篇Science，Vol3082005上的研究论文

Solar Wind Origin in Coronal Funnels : An Introduction of the Article Published in Science , Vol 308 , 2005

OH的同位素追踪显示大多数的氢来自于太阳风。

And the OH 's isotopic signature indicates that much of the hydrogen came from the solar wind .

但是它同样会被太阳风吹拂并趋向于拖延X星的运动。

But it is also blown about by the solar wind and tends to trail the moving Planet X.

行星际闪烁功率谱的Fresnel现象与太阳风速度

The Fresnel structure in interplanetary scintillation power spectrum and solar-wind velocity

太阳风里高能电子自发辐射的Langmuir波

Langmuir waves spontaneously emitted by energetic electrons in the solar wind

行星际闪烁（IPS）单站观测对太阳风速度的诊断

Single Station Interplanetary Scintillation Measurement to Diagnose Solar Wind Velocity

太阳风粒子密度的非线性Dirac方程。

The nonlinear Dirac equation of the particle density on the Solar Wind .

ACE探测到的是一股凶猛的太阳风，即不断从太阳中流出的带电粒子。

What ACE detected was a violent gust of " solar wind ", the constant flow of charged particles from the sun .

上面的图像是由X射线望远镜拍摄到的，如日出（？），冕洞之所以表现为黑暗，是因为炙热的发光气体将填补这些已蔓延的太阳风。

In images taken by X-ray telescopes , such as the one Hinode uses , coronal holes appear dark because the hot glowing gas which would otherwise fill them has spilled out in the solar wind .

当太阳风密度低且AE指数大于200nT时，地球同步轨道的电子强度会持续地增强。

When solar wind density was low and AE index greater than 200 nT , the 2 MeV electron flux at geostationary orbit will increase sustained .

唔，研究人员认为太阳风和辐射是“幕后黑手”，他们打算开展一项任务来找出原因何在。这项任务名为MAVEN——火星大气与挥发物演化任务（MarsAtmosphereandVolatileEvolutionMission）。

Well , researchers believe that solar wind and radiation is behind the theft , and they 're planning a mission to find out , called MAVEN : Mars Atmosphere and Volatile Evolution Mission

太阳风公司从YY公司以10美元的报价订购了一台机器。

Solarwind Company orders a machine from YY Company at a list price of $ 10 .

氢质子与太阳风（solarwind）中的氧结合产生了彗星尾巴中的水，而这些水又与彗星的自身电回路产生的可见光子（visiblephoton）组合。

The hydrogen protons combine with the oxygen in the solar wind to produce water in the comet 's tail ; which is comprised of visible photons ( coma ) generated by the comet 's electric circuit .

太阳风正负动压脉冲激发磁层ULF波的数值模拟

Numerical simulation of magnetospheric ULF waves excited by positive and negative impulses of solar wind dynamic pressure

由动力Alfven波沿磁场方向传播的扰动非线性方程，用量纲分析法导出太阳风中Alfven湍流谱。

The power spectrum of the kinetic Alfven turbulence is obtained from the nonlinear equations of the kinetic Alfven wave propagating along the magnetic field using dimensional analysis .

计算表明，K-H不稳定性确实能在太阳风-磁层耦合中起重要作用。

The calculations show that the Kelvin-Helmholtz instability can indeed play an important role in the coupling processes between the solar wind and the magnetosphere .

分析说明，当行星际磁场Bz分量出现南向扰动和太阳风速度增大超过500km/s时，地球磁层中常常发生磁暴/亚暴活动。

The analysis shows that geomagnetic storms / substorms can occur when the component B_z of the IMF is southward and the velocity of the solar wind increases to above 500 km / s.

采用二维理想MHD模型，分别在日球赤道面（二维二分量模型）和日球子午面（二维三分量模型）内研究太阳风中纯速度增幅扰动的演化。

Using an ideal two-dimensional MHD model , this paper investigates the evolution of a pure flow velocity enhancement disturbance in the solar wind in the heliospheric equatorial plane ( 2-D , 2-component model ) and the heliospheric meridional plane ( 2-D , 3-component model ) .

太阳风样本揭示了地球、月球与火星的同位素比例与太阳并不相同，表明星球的起源有着额外的原因。--KarenHopkin报道如果你曾对地球起源有过疑问，看起来答案是地球可能源自太阳风。

If you 've ever wondered where the Earth came from , the answer , it seems , is blowin " in the wind - the solar wind .

本文应用Helios飞船在0.3AU和1AU之间的高速太阳风质子和磁流涨落观测，同时考察了包括各种可能的加速和加热效应的高速太阳风动量方程和质子能量方程。

The momentum and energy equations for the high speed solar wind , which include all kinds of possible acceleration and heating processes , are examined simultaneously by using Helios ' observations of protons and MHD fluctuations in the high speed wind ranging from 1 AU to 0.3 AU .

结果表明，背景太阳风速度和ICME渡越时间并没有明显的相关性，在考虑了磁云通量管轴相对黄道面夹角的影响后相关性仍然不明显。

The results show that the ambient solar wind speed and the ICME transit time errors show little correlation , even after taking into account the angle of magnetic cloud flux tube to the ecliptic plane the correlation is still not obvious .

太阳风粒子速度分布不对称性的产生机制

A mechanism for the NON-GYROTROPIC distribution of the solar wind particles

太阳风高速流卡林顿周分布的演变

The Evolution of the Carrington Distribution of High-Speed Solar Wind Streams

太阳风质子束流密度的径向变化

Radial evolution of the proton beam density in the solar wind

高速太阳风中α粒子分布的形成

Formation of distribution of α particles in high speed solar wind

五矩二流太阳风等离子体特性的数值研究

Numerical study on properties of two-fluid Five-moment solar wind plasmas

太阳风中低频离子静电孤波

The electrostatic ion solitary waves with low frequencies in the solar wind

太阳风湍流和磁层亚暴的一种机制

Mechanism of magnetospheric substorm and the turbulence of solar wind