These events are known as coronal mass ejections or CMEs.

这些事件被称为日冕物抛射（CMEs）。

Solar flares and coronal mass ejections often occur near sunspots.

太耀斑和日冕物抛射经常发生在太附近。

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

另一种类型的太喷发被称为日冕物抛射，或 CME。

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

当被称为“日冕物抛射”的强烈太风涌向地球时，就会发生这种风暴。

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

也许当时发生了日冕物抛射。”

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

缺少太也意味着太耀斑以及它们更强烈的同胞-日冕物抛射的不存在。

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日，从暗条变成的日冕物抛射飞出了太。

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

星的日冕物抛射可能会导致电产品的瘫痪，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.

来自太的日冕物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。

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

大约一两天后，太风暴中最大的一部分会抵达地球，这叫日冕物抛射。

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

太的强磁能是太耀斑和被称为日冕物抛射的等离体爆发的来源。

These explosions are known as coronal mass ejections.

这些爆炸被称为日冕物抛射。

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

- 以下是更具爆炸性的日冕物抛射是如何发生的。

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

这是一种称为日冕物抛射或 CME 的现象。

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

日全食是科学家试图更好地了解日冕物抛射的一种方式。

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

名为日冕物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.

炽热的等离体在太内部移动，产生磁场，进而可以产生太、太耀斑和日冕物抛射。

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

尽管有一些耀斑不会导致日冕抛射，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，比如日冕物抛射。