英语释义

• a stream of protons moving radially from the sun

片语

solar-wind parameters太阳风参数

Solar wooden wind mill太阳能木制风车

solar r wind太阳风

solar and wind energy太阳能和风能

Solar and Wind Power太阳能及风力发电技术

Solar and wind power generation太阳能和风能发电

TYF太阳风（品牌名）

solar-wind power太阳能发电

Solar & wind energy(Solar)人名；(法、英、意、西、塞、捷)索拉尔

solar polar wind极区太阳风

英汉例句

• effects stemming from theearth「s atmosphere, from ocean tides and from the solar wind of chargedparticles were all found to be too small to explain the spacecrafts」 extravelocity.

  源自地球大气的影响，来自海洋潮汐和带电粒子的太阳风的影响都被发现小的不足以解释飞行器的额外速度的产生。

• 「when the solar wind blows out plasma it too causes a bubble: the heliosphere,」 he explains.

  他解释说：「当太阳风释放出等离子体时，它也会制造出一个泡泡：日光层。」

• the sweap solar wind experiment will count the electrons, protons and helium ions in the solar wind and measure their properties.

  sweap太阳风实验将计算太阳风中的电子，质子及氦离子的数量，并且测量这些粒子的性质。

• instead, the solar wind and the sun’s uv radiation give an electric charge to atoms and particles in mars outer atmosphere.

  相反，太阳风与太阳的紫外线辐射给予火星大气外侧的原子和粒子一个电荷。

• solar wind samples reveal that earth, the moon and mars have different isotopic ratios than the sun, indicating some additional wrinkles in the planetary origin scenario.

  对太阳风进行检测发现，太阳的同位素比例与地球、月球和火星不同，说明还有其他的因素参与了行星的起源。

• auroras happen when ions in the solar wind collide with atoms of oxygen and nitrogen in the upper atmosphere.

  极光的出现缘于太阳风离子与高层大气中的氧氮原子的碰撞。

• this coincidence enabled scientists to make giant strides in understanding the interaction of the solar wind with jupiter.

  这个巧合使科学家能够取得了认识太阳风与木星相互作用的巨大进展。

• the solar wind fluctuates in strength, but is prevented from entering both when it is strong and when it is weak.

  虽然太阳风的强度是波动的，电离层仍可以在太阳风强有力的时候阻止它穿过。

• the rate at which the solar wind transfers energy to the magnetosphere can vary widely, but what determines the rate of energy transfer is unclear.

  太阳风将能量转化至磁气圈的速率变化很大。但是目前为止，我们仍不清楚到底是什么在决定着这种传送速率。

• particles in the solar wind collide with gas molecules high in earth’s atmosphere, transferring some of their energy and boosting the molecules「 electrons into an ‘excited’ state.

  太阳风暴中的粒子和地球大气中的气体分子相撞，粒子把自身的一部分能量转化并灌注到气体分子的电子中，使分子中的电子呈现出一种激发即高能的状态。

• the e-sail would thus catch the solar wind like some huge dandelion seed that is blown aloft by terrestrial breezes.

  该电子帆像一些被吹起的蒲公英种子那样搭乘太阳风。

• the waves of damp and dry conditions suggest water is created on the moon every day, when hydrogen nuclei in the solar wind slam into oxygen-rich silicate minerals on the moon」s surface.

  潮湿和干燥条件的交替波动表明，月球上每天都在生成水——太阳风中的氢原子核与月球表面富含氧的硅酸盐矿物相撞而成。

• the first critical step is to understand how the energy gets transferred from the solar wind to the magnetosphere.

  首要的问题是，我们得搞清楚能量是如何从太阳风转化到磁气圈中去的。

• hydrogen atoms are more abundant than either helium or oxygen but their low mass means they are easily swept aside by the high-speed solar wind and can’t readily be detected.

  福斯勒指出氢原子数量比氦原子或氧原子数量要多得多，但是它质量很小，很容易被太阳风吹散，从而不能被稳定地观测到。