At about 3,000 kilometers above the surface, we reach the chromosphere, the second layer of the sun.

在距离表面约 3000 公里的地方，我们会到达色球，第二层的太阳。

Now you can see the pearly glow of the sun’s corona and the pink and red light from the hydrogen gas of the chromosphere.

现在您可以看到日冕发出的珠般的光芒，以及色球层氢气发出的粉红和红光。

They also funnel high energy particles down to a layer of the Sun called the chromosphere, where they quickly transfer their energy like a cue ball striking the rack in the game of billiards.

它们还能集合成高能粒子，掉进太阳的光化层，在那这些高能粒子快速的转化其能量，像台球中开球时用母球撞击一堆目标球一样。