Plasmas aren't just beautiful, celestial phenomena, though.

但是等离子体不仅仅是绚丽的天空现象。

It shoots out a plasma blade that's hotter than 5,000 degrees Fahrenheit.

它射出的等离子体刀片的温度超过5000华氏度。

To get the fiery ball of plasma, the grape needs some preparation.

想得到等离子体的火球，这个葡萄要经过加工。

The sun has hurled plasma and other magnetic activity toward the Earth.

太阳向地球发射了等离子体并进行了其他磁活动。

Another such blast drives off solar material called plasma.

另一种这样的爆炸会释放出称为等离子体的太阳物质。

You could just get a bunch of iron and plasma and put it together.

你可以买大量的铁和等离子体，然后将它们组装起来。

Plasma is the fourth state of matter after solids, liquids, and gases.

等离子体是继固体、液体和气体之后的第四种物质状态。

They'll create magnetic fields strong enough to contain the superhot plasma created by fusion.

超导体能制造出足够强大的磁场，控制住聚变产生的超高温等离子体。

Plasma consists of charged particles that produce powerful magnetic fields.

等离子体由电粒子组成，这些电粒子又形成强力的磁场。

When the plasma reaches the surface, it cools.

当等离子体到达表面时，它就会降温。

You had a jet of plasma traveling very fast that impacted on the magnetopoles-that's the boundary of our magnetosphere.

移动速度极快的等离子体射流撞击磁极——也就是地球磁层的边界。

When this plasma reaches the Sun's surface, their magnetic fields do too.

当这个等离子体到达太阳表面时，它们的磁场也会发生变化。

Parker's orbit takes it through the sun's corona to sample where corona plasma detaches to become solar wind.

帕克探测器的轨道使其可以穿过太阳的日冕层，在那里，日冕等离子体会分离形成太阳风。

And it vibrates like a drum when jets of charged particles from the sun, called plasma, crash into it.

当称为等离子体的来自太阳的电粒子喷射进磁层时，磁层就会像鼓一样振动。

It's an infernal sphere, of mostly hydrogen and helium, superheated into a plasma, that burns at millions of degrees.

它是一颗地狱般的星球，大部分是氢和氦，它们在高温下成为等离子体，在数百万度的高温下燃烧。

The liquid convects, and this motion generates magnetic fields, similar to the way plasma in the Sun generates magnetic fields.

这些液态物质的对流会产生磁场，类似于太阳中的等离子体产生磁场的方式。

Few materials could handle the scorching plasma of our sun.

很少有材料能够承受太阳灼热的等离子体。

This can energize the plasma even further, heating it up.

这可以给更远的等离子体供给能量，使其升温。

Plasma on the Sun's surface can flow along these magnetic loops, too.

太阳表面的等离子体也可以沿着这些磁环流动。

In a CME energy from a flare flings a blob of highly charged radioactive plasma out of the solar atmosphere.

在一个CME里，耀斑发出的能量会将一堆高电荷辐射性等离子体抛出太阳的大气层。