因为极紫外线的波长在100å到1000å之间(注一)是会被大气中的臭氧层吸收,可是氢原子的 来曼系 ( Lyman series )都是落在紫外线区域,宇宙大部分成分又是氢,对于研究宇宙的天文学家,臭氧层似乎不太讨他们喜欢。
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solar emission of Lyman series 太阳莱曼系辐射
以上来源于: WordNet
We can think about the Lyman series.
我们可以来看看莱曼系。
We can think about the Lyman series, which is 1 where n equals 1. We know that that's going to be a higher energy difference, so that means that we're going to be in the UV range.
我们可以来看看Lyman系,也就是n等于,我们知道它的能量差更大,所以它在紫外光区内。
We can think about the Lyman series, which is 1 where n equals 1. We know that that's going to be a higher energy difference, so that means that we're going to be in the UV range.
我们可以来看看Lyman系,也就是n等于,我们知道它的能量差更大,所以它在紫外光区内。
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