J.J. Balmer, who was a school teacher in the 1800s, was the first to describe these lines that could be seen from hydrogen.
J.J. Balmer,在19世纪是一名教师,他是第一个描述这些可以从氢气中看到的线条的人。
Some are very characteristic absorption lines: some for hydrogen, some for calcium, some for silicon, some for magnesium and so on.
有些是非常,典型的吸收线:,有些代表氢元素,有些代表钙元素,有些代表硅元素,有些代表镁元素等等。
So, even though the lines were wrong, he says, no, that is hydrogen.
所以,即使那光线是错误的,他说,不,它就是氢。
Payne said technicians found that seals on the hydrogen vent lines were out of alignment and they installed new ones to fix the leaks.
VOA: standard.2009.06.16
First there was the observation by Michelson who back in the late 1880s had done very precise interferal metric measurements of the hydrogen lines and had observed that the 656 nanometer line 3 associated with the transition of n equals 3 to n equals 2 was, in fact, a doublet.
首先是麦克逊,在1880年底的观察,他以公制单位对氢原子的光谱线,作了准确的,无其他因素干扰的,测量,发现当n值由3变为2时,会同时得到波长为656纳米的谱线3,实际上是有两条线。
In 1896, Charles Pickering from Harvard found a series of lines in starlight which he attributed to hydrogen, even though they did not fit Balmer.
在1896年,来自哈佛的查尔斯皮克林发现,一系列的星光,他认为那是氢的作用,虽然它们与巴尔末理论不符。
应用推荐