对于暗物质，宇宙微波背景辐射才不管你的冷热。
For dark matter, the cosmic microwave background doesn't care whether you're hot or cold.
但批评他的工作的这几组人认为宇宙微波背景辐射并不是这样的。
But the groups who are critical of his work say that this is not what the cosmic microwave background is like.
这是基于宇宙微波背景辐射和物理学公理的联合推论。
This is an combined inference derived from Axiom of Physics and observation of CMBR.
但是，我们不能像利用微波背景辐射这般准确地做到这点。
But we couldn't do it as accurately as we can from the fluctuations in this microwave background.
宇宙微波背景辐射(CMB)也为大爆炸理论提供了有力的线索。
The cosmic microwave background - called the CMB for short - also provides evidence to back up the Big Bang theory.
然而，对宇宙微波背景辐射温度的测量显示宇宙的结构也许有某种系统的规律。
However, measurements of the cosmic microwave background radiation temperature suggest that its structure may have some systematic order.
介绍了有关宇宙微波背景辐射（CBR）观测和理论研究的最新进展。
The recent progress on observation and theory of the cosmic microwave background radiation(CBR) is presented in this paper.
文章对微波背景辐射的各向异性、偏振及宇宙电离的历史给出了评述性介绍。
We describe the basics of the cosmic microwave background radiation (CMB), and the physics of its anisotropy and polarization.
他在黑体和宇宙微波背景辐射各向性的研究跟宇宙起源的观点有许多想通之处。
His work in black body form and anisotropy of the cosmic microwave background radiation CEMENTED our understanding of the origin of the universe.
科学家将研究分析微波背景辐射中几百万分之一的温度变化，看是否能从中找出它的这些特性。
They will examine temperature variations in the microwave background amounting to a few millionths of a degree, to see whether they can discern such features in it.
卡什林斯基和同事们是在研究星系团气体与宇宙微波背景辐射之间相互作用时首次注意到黑暗流的。
Kashlinsky and colleagues first noticed the dark flow when studying the way gas in galaxy clusters interacts with the cosmic microwave background radiation.
南极望远镜2007年开始工作。它的作用是观察宇宙微波背景辐射，这是宇宙大爆炸的“余辉”。
The South Pole Telescope, which began scientific observations in 2007, surveys the sky for cosmic microwave background radiation, the "afterglow" of the Big Bang.
这个奖授予宇宙微波背景辐射的黑体谱形和各向异性的发现，强有力地支持了大爆炸宇宙学。
It was awarded for the discovery of the blackbody spectrum and anisotropy of the cosmic microwave background radiation which strongly supports the big bang theory of cosmology.
这个奖授予宇宙微波背景辐射的黑体谱形和各向异性的发现，强有力地支持了大爆炸宇宙学。
It was awarded for the discovery of the blackbody spectrum and anisotropy of the cosmic microwave background radiation, which strongly supports the big bang theory of cosmology.
微波背景辐射显示的宇宙高度的均匀性和各向同性说明，宇宙已经存在了约150亿年左右。
The high homogeneity and isotropy shown in the cosmic microwave background (CMB) prove that the universe has been in existence for around 15 billion years.
描绘宇宙微波背景辐射是很困难的，因为银河系本身在这些波长发射很多，使得背景辐射难以分离出来。
Mapping the cosmic microwave background is hard because the Milky Way itself shines quite brightly at these wavelengths, making the background hard to discern.
但WMAP却没能够发现这些高能量的光子，所以在宇宙微波背景辐射上那些星系的周围有些光子的亏损。
WMAP cannot detect these higher energy photons, so there should be a deficit of CMB photons around clusters.
当宇宙微波背景辐射通过星系团时，气体将其中光线散射开来，其方式类似于地球大气层散射星光而使一些星星貌似闪烁。
These gases scatter light from the cosmic microwave background radiation as it passes through the clusters, similar to the way Earth's atmosphere can scatter starlight, making some stars twinkle.
阿尔诺·彭齐亚斯和罗伯特·威尔逊在1965年发现了宇宙微波背景辐射，这使得大爆炸理论在科学界获得了广泛支持。
The theory of the big bang gained widespread support in the scientific community after Arno Penzias and Robert Wilson discovered cosmic microwave background radiation in 1965.
这一进展多半来自对大爆炸“余辉”——也就是为人所熟知的，名为“宇宙微波背景辐射”(CMB)的辐射能——的研究。
Much of the progress has come through studies of the afterglow of the big bang, radiation known as the cosmic microwave background (CMB).
近年来通过对“微波背景辐射”及遥远射电星系发出的射电波的观测表明，它们存在一与地球运动相关的各向异性。
Recent observations on microwave background radiation and distribution of distant radio galaxies demonstrate that there exists dipole anisotropy in relation to the motion of the Earth.
彭罗斯博士还预测了另一种不均匀性形态的存在---这就是宇宙“大圈”， “宇宙微波背景辐射”在“大圈”中略显均与性。
Dr Penrose, though, predicts another form of irregularity—great circles in the sky where the microwave background is slightly more uniform than it should be.
宇宙微波背景辐射有很多“热点”和“冷点”，但都没有稳定在某一水平，从表面上看，是不应该出现这样的情况的。
The CMB radiation has many hot and cold spots in it, but none above a certain size. On the face of it, there is no reason why this should be so.
欧洲航天局最近开始投运的普朗克空间望远镜，在它能画出更为灵敏的宇宙微波背景辐射的天体图时，就可能解决这个问题。
The European Space Agency's recently launched Planck space telescope might settle the issue when it makes the most sensitive maps yet of the CMB.
威尔逊和彭齐亚斯捕捉人造卫星上反弹回来的无线电波的天线时不经意地发现了宇宙微波背景辐射，而这正是宇宙大爆炸的物理性证据。
And Wilson and Penzias discovered the cosmic microwave background radiation, physical evidence for the Big Bang, while fiddling with an antenna designed to catch radio waves bouncing off satellites.
彭齐亚斯和威尔逊发现了宇宙大爆炸理论的有力证据——微波背景辐射，其原意只不过是架设一台用以接受卫星信号的天线。
And Wilson and Penzias discovered the cosmic microwave background radiation, physical evidence for the Big Bang, while fiddling with an antenna designed to catch radio waves bouncing off satellites.
研究宇宙微波背景辐射-就是大爆炸以后残留下来的辐射-的科学家说，他们已经发现一些发生在离这里二十几亿光年以外的奇怪的事情。
Scientists studying the cosmic microwave background - that's the radiation leftover from the Big Bang - say they've detected something strange happening couple of billion light years from here.
从威尔金森微波各向异性探测器(WMAP)得来的数据显示出，细微温度变化是在宇宙微波背景辐射移动通过银河星系团气体时产生的。
Data from the Wilkinson microwave Anisotropy Probe (WMAP) can show the minute temperature changes created as the cosmic microwave background radiation moves through gases in galaxy clusters.
一个像号角的宇宙也许会令人感到很惊奇，不过它能够解释一些令人费解的宇宙微波背景辐射的数据——这是大爆炸后残留的宇宙辐射。
A universe shaped like a Bugle may sound odd, but it could help explain some puzzling observations of the cosmic microwave background radiation: the relic radiation left over from the big bang.
一个像号角的宇宙也许会令人感到很惊奇，不过它能够解释一些令人费解的宇宙微波背景辐射的数据——这是大爆炸后残留的宇宙辐射。
A universe shaped like a Bugle may sound odd, but it could help explain some puzzling observations of the cosmic microwave background radiation: the relic radiation left over from the big bang.
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