This is what people are talking about when they refer to the dangers of solar storms and coronal mass ejections, which are essentially when the Sun spews out plasma that, along with its embedded magnetic field, can reach Earth.

这就是人们口中的太阳风暴和日冕物质抛射的危险问题，本质上是太阳喷出等离子体，连同它的嵌入磁场，到达地球。

These events are known as coronal mass ejections or CMEs.

这些事件日冕物质抛射（CMEs）。

Another type of solar eruption is called a coronal mass ejection, or CME.

另一种类型的太阳喷发日冕物质抛射， CME。

Such storms happen when strong surges of solar winds called coronal mass ejections reach Earth.

当“日冕物质抛射”的强烈太阳风涌向地球时，就会发生这种风暴。

And maybe at that time, there is what is known as a coronal mass ejection.

也许当时发生日冕物质抛射。”

Then, there are Coronal Mass Ejections, which rip millions or billions of tonnes of plasma from the Sun's atmosphere, catapulting it through the Solar System at speeds of up to 9 million kilometres per hour.

然后就产生冠状物质的喷射，它用900万千米每小时的速度弹射通过太阳系，夺走太阳大气层的十百万的等离子体。

Although magnetic field lines are invisible, we know they exist on the Sun by looking at features called " coronal loops" and " prominences" rising up into the solar atmosphere.

尽管磁力线看不见，我们却知道其存在于太阳上，通过观察“冕环”和“日珥”的特殊现象，“冕环”和“日珥”会一路上升到太阳的大气层。

The Advanced Space-Based Solar Observatory, or the ASO-S, will provide critical insights on the two most violent activities of Earth's closest star: solar flares and coronal mass ejections, along with the powerful radiation and complex magnetic fields they generate.

先进天基太阳天文台将对地球上最近的恒星——太阳上两类最剧烈的爆发现象提供关键的见解：太阳耀斑和日冕物质抛射，以及它们产生的强大辐射和复杂磁场。

The beauty of nice coronal mass ejections is that we get to have an astronomical event basically come to us from space that's visible to the naked eye.

日冕物质抛射的美妙之处在于，这是一个我们可以用肉眼看到太空的天文事件。

It consists of solar wind, solar flares and coronal mass ejections, which are these giant bubbles of plasma and magnetic fields from the sun that send high speed particles into space.

它由太阳能风能、太阳耀斑及日冕物质抛射组成, 就是这些来自太阳的巨大泡沫等离子体及磁场将高速粒子射入太空。

We can see big explosions things called solar flares or coronal mass ejections and that's why we like to look at it in all these different wavelengths

我们可以看到大爆炸，太阳耀斑日冕物质抛射的东西，这就是什么我们喜欢用不同的波长来观察它的原因。

All that magnetic activity also leads to solar flares, which are bright bursts of radiation, and coronal mass ejections, or CMEs, which spit magnetized plasma out into space.

所有这些磁活动还会导致太阳耀斑，而这是明亮的辐射爆发以及日冕物质抛射（CME）——将带有磁性的等离子体喷射到太空中。

But we are not fully protected from what scientists call Coronal Mass Ejections. These are strong storms that can happen on the sun's surface.

但我们不能完全避免科学家所说的“日冕物质抛射”的伤害，这种强风暴发生在太阳的表面。

" We can actually see the spacecraft flying through coronal structures that can be observed during a total solar eclipse, " Raouafi said.

" 我们能够真切地看到该航天器穿过日冕结构，这种结构在日全食时期间可以观测到。"

Extreme solar storms called " coronal mass ejections" can erupt into space almost without warning, unleashing huge waves of charged particles.

名日冕物质抛射能的极端太阳风暴毫无预警地向宇宙爆发，释放巨大的带电粒子波。

Scientists call this the coronal heating problem and evidence for this was first uncovered during an eclipse in the 1800s.

科学家们之日冕加热问题，这方面的证据是在 19 世纪的一次日食中首次发现的。

This is called a coronal mass ejection, and it results in a geomagnetic storm when it arrives at the Earth.

这日冕物质抛射，当它到达地球时会导致地磁风暴。

The sun's strong magnetic energy is the source of solar flares and bursts of plasma known as coronal mass ejections.

太阳的强磁能是太阳耀斑和日冕物质抛射的等离子体爆发的来源。

An absence of sunspots also means an absence of solar flares and their more violent siblings, coronal mass ejections.

缺少太阳黑子也意味着太阳耀斑以及它们更强烈的同胞-日冕物质抛射的不存在。

Coronal objections from stars have the potential to cripple technology and even burn off parts of the planet's atmosphere.

恒星的日冕物质抛射可能会导致电子产品的瘫痪，并且甚至会引燃行星的部分大气层。