What is the translation of " 宇宙微波背景 " in English?

Noun
cosmic microwave background
宇宙 微波 背景
CMB

Examples of using 宇宙微波背景 in Chinese and their translations into English

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因探测到“宇宙微波背景辐射”而获得诺贝尔奖。
Prize motivation:"for their discovery of cosmic microwave background radiation.".
宇宙微波背景辐射正是在此期间产生。
The photons of the cosmic microwave background radiation originate at this time.
宇宙微波背景辐射”正是在此期间产生的。
The photons of the cosmic microwave background radiation originate at this time.".
他的研究兴趣为宇宙微波背景
His current research interests lie in the Cosmic Microwave Background.
在19世纪60年代,科学家们发现了宇宙微波背景辐射(CMBR)-它是空间中来自宇宙大爆炸的辐射。
In the 1960s, scientists discovered Cosmic Microwave Background Radiation(CMBR)- traces of radiation in space from the Big Bang.
宇宙微波背景光谱可以区分这两种,因这两种类型的扰动会产生不同的峰值位置。
The CMB spectrum is able to distinguish these two because these two types of perturbations produce different peak locations.
根据标准的宇宙学模型,相对于宇宙微波背景星系团的运动应该是随机分布在所有方向。
According to standard cosmological models,the motion of galaxy clusters with respect to the cosmic microwave background should be randomly distributed in all directions.
宇宙微波背景测量不是直接测量局部膨胀,而是通过一个模型――宇宙模型来推断。
The Cosmic Microwave Background measurements don't measure the local expansion directly, but rather infer this via a model- our cosmological model.
宇宙微波背景光谱可以区分这两种,因这两种类型的扰动会产生不同的峰值位置。
The CMB spectrum can distinguish between these two because these two types of perturbations produce different peak locations.
我们还把我们的测量结果与“普朗克”(Planck)宇宙微波背景实验提供的独立测量结果作了比较。
We also compare ourmeasurement with the independent measurement provided by the Planck CMB experiment.
宇宙微波背景是浅,是最远的距离我们,我们可以看到,他说:Riess。
The cosmic microwave background is the light that is the furthest away from us that we can see,” said Riess.
当然,我们无法看到宇宙微波背景之外,因为早期宇宙炽热致密,使其处于不透光的状态。
Of course we can't see beyond the cosmic microwave background, because the early universe was so hot and dense that it wasn't transparent.
WMAP观察测五段频率,允许测量并消去前景污染(源自银河系及银河系外)的宇宙微波背景
The WMAP observes in five frequencies, permitting the measurement and subtraction of foreground contamination(from the Milky Way andextra-galactic sources) of the CMB.
尽管我们无法直接观测到宇宙微波背景之外,但我们对这之前的时间知道得不少。
Despite our inability to directly observe beyond the cosmic microwave background, we do know quite a bit about the time before it.
但是考虑到我们在宇宙微波背景下的波动图,我们可以得出这样的结论:这些温度从未达到过。
But given the map of the fluctuations we have in the Cosmic Microwave Background, we can conclude those temperatures were never achieved.
今天,它出现在光谱的微波部分,被称为宇宙微波背景
Today, this shows up in the microwave portion of the spectrum,and is known as the Cosmic Microwave Background.
关于宇宙历史的非凡信息来源在于这种“化石”辐射,称为宇宙微波背景(CMB)。
An extraordinary source of information about the universe's history lies in this“fossil” radiation,called the cosmic microwave background(CMB).
大爆炸的回声在整个天空形成了一个微波信号,被称为宇宙微波背景
The echoes of the Big Bang form a microwavesignature across the entire sky that is called the cosmic microwave background.
年至2013年,普朗克卫星观测到的遗物辐射,有时也被称为宇宙微波背景(CMB)辐射。
Between 2009 and 2013, the Planck satellite observed relic radiation,sometimes called cosmic microwave background(CMB) radiation.
我们现在可以寻找这些原初引力波,它们从某种程度上来讲类似于宇宙微波背景辐射。
Now we can look for these primordial gravitational waves,which are kind of analogous to the cosmic microwave background radiation.
如果你通过研究大爆炸的余辉来计算它,它与从宇宙微波背景计算它是完全不同的。
If you calculate it by studying the afterglow of the Big Bang,it's a completely different value from calculating it from the cosmic microwave background.
特别是,他们将使用当前和未来欧洲空间局测量宇宙微波背景辐射和引力波的任务数据。
In particular, they will use data from current andfuture ESA's missions measuring cosmic microwave background radiation and gravitational waves.
大质量的蓝星嵌在气体和尘埃的细丝中,而宇宙微波背景(CMB)显示在外层边缘。
The massive blue star is embedded within filaments of gas anddust, while the cosmic microwave background(CMB) is shown on the outer edges.
一种方法基于我们的实验可以看到的最远辐射来计算扩展,称为宇宙微波背景
One method calculates the expansion based on the farthest radiation that our experiments can see,called the cosmic microwave background.
因为水蒸气吸收微波,干燥的气候使已经稀薄的大气层传递出更微弱的宇宙微波背景辐射。
Because water vapor absorbs microwaves, the dry climate allows the already thinatmosphere to transmit even more of the faint cosmic microwave background radiation.
宇宙微波背景的发现,以及黑洞的观测,支持这些结论。
The discovery of the cosmic microwave background, and observations of black holes, support these conclusions.
但是这比依靠宇宙微波背景来测量的结果要高出7%。
However, it is about 7% higher than measurements that rely on cosmic microwave background for measurement.
宇宙微波背景的波动显示了一个宇宙,其尺度延伸到可观测宇宙的地平线上。
The fluctuations in the cosmic microwave background show a Universe with scales that extend up to and beyond the horizon of the observable Universe.
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