solar wind的例句大全

The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere.

从太阳风传来的磁场能量，彻底改变了磁层形状。

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

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

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Speed dependence of solar wind mass flux in the ascending phase of solar activity

太阳活动上升期源表面太阳风质量流量的速度关系分析

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So solar wind transport into magnetosphere is one of the most important problems in magnetosphere research.

因此，太阳风向磁层的传输是磁层物理研究的一个非常重要的问题。

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Gargantuan aurora's with no solar wind?

巨大的极光会没有太阳风？

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

太阳风正负动压脉冲激发磁层ULF波的数值模拟

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Polar ionosphere is especially structured and coupled with magnetosphere via convection electric field, particle precipitation and field-aligned current. It plays an important role in the coupling processes among the solar wind, magnetosphere, ionosphere and thermosphere.

极区电离层通过对流电场、粒子沉降和场向电流与磁层紧密耦合在一起，在太阳风-磁层-电离层以及热层耦合过程中起着重要作用。

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the results show that the magnetosphere does not act as the half-wave rectifier to the solar wind effects, hence the classical recon-nection scheme of the magnetosphere is proposed to be somewhat modified.

从耦合方程出发讨论了磁层对太阳风作用的响应，证明磁层不是起半波整流器作用，从而表明经典的重联理论应有所修改。

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Solar wind: What you do there are a broom, I can sweep clean for you

太阳风：请问，您这里有扫帚吗，我可以替你打扫打扫

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2-dimensional structure of solar wind speed on the source surface

太阳风速度的源表面二维结构

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

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。

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Energy transport from the solar wind to equatorial electrojet area

太阳风能量向赤道电离层的传输

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The more active the Sun, the stronger the solar wind.

太阳活动越剧烈，太阳风越强烈。

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The solar wind-magnetosphere-ionosphere coupling during magnetic storm

磁暴期间太阳风-磁层-电离层间的耦合过程

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In this review we summarize the recent advances in coronal physics. Some results of investigations are discussed such as the coronal structures, energy balance, theory of coronal heating mechanisms and solar wind streams.

本文总结了日冕物理研究的最新进展，讨论了有关日冕的结构，能量平衡，日冕加热机制的理论以及太阳风等的某些研究成果。

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It is shown that the acceleration of high speed solar wind in the coronal hole due to the whistler waves is very important.

结果表明，哨声波是引起冕洞高速太阳风加速的重要原因。

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We propose that the future forecasting of the physical conditions that the violent solar disturbance causes at the earth by propagating in solar wind depends heavily on the numerical method.

未来预测太阳剧烈扰动所造成的行星际风暴到达地球空间的状态势必借助于数值方法。

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A complex coupling system is formed by the solar wind, magnetosphere and ionosphere in geospace. And an important process in geospace that is still not fully understood is the plasma transport between the plasmasphere and the ionosphere during different interplanetary disturbance and geomagnetic condition.

太阳风-磁层-电离层组成了地球空间的一个复杂的耦合体系，基于不同行星际条件或地磁条件下，等离子体层和电离层间物质输运机制仍未弄明。

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Under the quiet solar wind condition, the dayside magnetopause is at about 10R_E from the center of the Earth.

向日面磁层顶在平静太阳风条件下，处于10RE（RE为地球半径）左右。

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The researchers note that similar chemistry could be at work on Mercury, large asteroids and other airless bodies that endure the full blast of the solar wind.

研究人员指出类似的化学反应在水星、大型行星以及其他空气稀薄并能承受太阳风猛烈冲击的星体上也有发生。

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