These events are known as coronal mass ejections or CMEs.

这些事件被称为冕物质抛射（CMEs）。

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

类型的太喷发被称为冕物质抛射，或 CME。

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

也许当时发生了冕物质抛射。”

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

缺少太黑子也意味着太耀斑以及它们更强烈的同胞-冕物质抛射的不存在。

A coronal mass ejection from a filament lifted off the sun on March 3rd, according to the U.S. government.

据美国政府称，3月3，从暗条变成的冕物质抛射飞出了太。

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

恒星的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。

Coronal mass ejections from the Sun are perhaps the most dangerous threat you've never heard of.

来自太的冕物质喷射也许是你从未听说过的最危险的东西。

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

科学家们称之为冕加热问题，这方面的证据是在 19 世纪的食中首发现的。

About a day or two later, the biggest part of the storm arrives. It is called a coronal mass ejection.

大约两天后，太风暴中最大的部分会抵达地球，这叫冕物质抛射。

These explosions are known as coronal mass ejections.

这些爆炸被称为冕物质抛射。

Here's how the more explosive coronal mass ejections happen.

- 以下是更具爆炸性的冕物质抛射是如何发生的。

This is a phenomenon known as a coronal mass ejection, or CME.

这是称为冕物质抛射或 CME 的现象。

A total eclipse is one way scientists try to better understand coronal mass ejections.

全食是科学家试图更好地了解冕物质抛射的方式。

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

名为冕物质抛射能的极端太风暴毫无预警地向宇宙爆发，释放巨大的带电粒子波。

Hot plasma moves inside the Sun, creating magnetic fields, which in turn can create sunspots, solar flares, and coronal mass ejections.

炽热的等离子体在太内部移动，产生磁场，进而可以产生太黑子、太耀斑和冕物质抛射。

Though some flares do not result in coronal ejections, when they do, the star spews out hot, radiated clouds of plasm.

尽管有些耀斑不会导致冕抛射，当它们发生时，它们会抛射出炽热的带有辐射的等离子云。

Well, for that we can blame the Sun, specifically, its solar winds and solar storms, like coronal mass ejections.

好吧，为此我们可以责怪太，特别是它的太风和太风暴，比如冕物质抛射。

Coronal ejections usually occur during a sun flare, which is a sudden increase in energy output on the surface of a star.

冕抛射通常发生在太耀斑期间，是恒星表面能量突然的爆发。

" 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冕结构，这结构在全食时期间可以被观测到。"

But every now and then, a large coronal mass ejection can overwhelm our defenses, disabling satellites and causing power outages.

但时不时地，大规模的冕物质抛射会压垮我们的防御系统，使卫星瘫痪并导致停电。