This article demonstrates the method of simulating the calibration curve of hydrogen atomic spectrum using the Lorentz dispersion relation.
本文介绍了如何利用折射率的洛伦茨色散关系拟合氢原子光谱实验的定标曲线的方法。
He had a tube with electrodes potted in it filled with atomic hydrogen. And by applying a voltage, he was able to get the gas to glow.
他有一根装着电极的管子，里面充满了氢原子。通过施加电压，他能够使气体发光。
But, it could be not just atomic hydrogen.
但是，它不能仅仅是原子氢。
We saw the Schr?dinger equation for atomic hydrogen, but you can write it for more complex systems.
我们看过原子氢的薛定谔方程，但其实我们能把他用在更复杂的体系。
They discovered a first order phase transition, a discontinuity, in liquid hydrogen between a molecular state with low conductivity and a highly conductive atomic state.
他们发现了一个不连续的一级相变，这个相变是在液态氢低电导率的分子态和高电导率的原子态之间。
OK, atomic hydrogen, one proton, one electron.
原子氢，单个质子，单电子。
Hydrogen, we can first draw in our atomic electrons.
氢原子，我们可以先画出原子电子。
That is the electron in its lowest orbit, to the nucleus of atomic hydrogen.
那就是氢原子原子核外电子，最低轨道到情况。
It is a double column, You can see, it starts with hydrogen and goes to mercury in ascending order of atomic mass.
双纵栏，你们看到，从氢开始，然后到水银，按原子质量的升序排列。
In other words, just want to know where the electron is somewhere within the shell radius of the ground state of atomic hydrogen anywhere.
换言之，我只是想知道，电子在哪，可以在氢原子基态下的半径，里面的任何地方。
He measured the line spectra of atomic hydrogen.
测量了氢原子的线光谱。
H We've been talking about atomic hydrogen, h.
我们讨论的原子氢。
This is the 1s. And, just to be clear, this is the 1s atomic orbital in atomic hydrogen.
说清楚，这是原子氢的1s原子轨道。
Now, as they report in Nature Physics, the researchers have used their device to preserve anti-hydrogen for 16 minutes (aeons in atomic-physics terms).
现在，研究人员在自然物理杂志上发表的报告称，他们已经利用设计的装置将反氢子存在时间延续到了16分钟。 （在原子物理术语上相当于亿万年）。
I just burst in now, I look up there and go that's atomic hydrogen.
我现在突然出现，我在这抬头看看然后离开，那就是氢原子。
His discoveries, which won him the Nobel prize, led to the caesium atomic clock and the hydrogen maser.
这一获得诺贝尔奖的发现产生了铯原子钟和氢微波激射器。
But it is interesting. Let's just, for an order of magnitude say what happens for ground state electron in atomic hydrogen?
但行星模型其实挺有趣的，按照重要的先后顺序，我们来猜想一下，氢原子中的基态电子会发生些什么？
That is the ground state energy of atomic hydrogen.
同时也是氢原子基态的能量值。
This is the diagram taken right from your text, there are the two electrodes coming in and this is atomic hydrogen in the gas tube.
这是从教科书上复制下来的图表，这里有两个电极进来，这是气体管中的氢原子。
Take the fattest marking pen you have, scratch that out and replace it with atomic hydrogen.
用你最粗的笔把它划掉，再用氢原子代替它。
In atomic hydrogen, is it fast? Is it slow?
在氢原子里，速度是快还是慢？
It begins with Maarten Schmidt who hypothesized that star formation rate (SFR) was related to the surface density of atomic hydrogen gas in the cloud.
最早是MaartenSchmidt猜测恒星形成率(SFR)与云层中氢原子气体密度有关。
The results show that hydrogen reduces the fracture activation energy by 74%, that is, atomic binding force decreases.
结果表明：氢的存在使断裂激活能约降低74%。这说明其减弱了原子间键合力。
A couple of other things about hydrogen: hydrogen also, like other elements, has isotopes and we already saw that in 1766, Cavendish isolated atomic hydrogen and enunciated some of its properties.
一些关于氢的东西：，氢气，就像其他元素一样，有同位素，人们在1766年就发现了这一点，卡文迪许分离出原子氢，并且阐述了它的一些性质。
All methods are primarily based on the generation of large amounts of atomic hydrogen and carbon radicals.
所有的方法首先要以大量原子态氢和碳基的产生为基础。
An isotope of hydrogen with one proton and one neutron in the nucleus having an atomic weight of 2.04.
氢的一种同位素，在其原子核内有一个质子和一个中子，其原子重量为2.04。
Translation: We should keep in mind these days when scientists of the older generation successfully developed the atomic and hydrogen bombs.
我们应该记住老一辈科学家们为成功研制“两弹”而努力奋斗的那些日日夜夜。
A hydrogen molecule consists of only two hydrogen atoms with the same atomic weight.
氢分子仅由两个原子量相同的氢原子组成。
Based on available frequency standards: one prototype laboratory model of cesium clock, three hydrogen clocks and several (2-6) rubidium clocks, the SO atomic time scale has been established.
利用我们现有的标准，一台试验型实验室铯束标准，三台氢原子钟以及若干台(2 -6)铷气泡标准来建立原子时尺度。
The ATA can observe a wide range of wavelengths, so it can check stars in the foreground for ETI signals while it watches background galaxies for clouds of atomic hydrogen.
ATA能够观察广泛的波长，因此可以检查在氢原子云层的星系团背景下的前景ETI信号。
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