Examples of using 宇宙微波背景辐射 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。
宇宙微波背景辐射正是在此期间产生。
宇宙微波背景辐射”正是在此期间产生的。
先是发现于1965年的宇宙微波背景辐射。
The cosmic microwave background radiation was actually found in 1965.Combinations with other parts of speech
A彭齐亚斯和威尔逊首次发现宇宙微波背景辐射.
Penzias and Wilson discovered the cosmic microwave background radiation.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 宇宙微波背景辐射和宇宙学红移－距离的关系一同被视为大爆炸理论最好的证据。
The cosmic microwave background radiation and the cosmological redshift-distance relation are together regarded as the best available evidence for the Big Bang theory.宇宙正在膨胀，宇宙微波背景辐射的波长已经伸长。
The universe is expanding, and the wavelength of the cosmic microwave background radiation has stretched.普朗克将以前所未有的准确程度审视宇宙微波背景辐射，目的是检验关于早期宇宙以及宇宙结构来源的各种理论。
Planck will examine cosmic microwave background radiation, to a degree of accuracy never achieved before, to test theories of the early universe and the origin of WMAP花费9年所制成的宇宙微波背景辐射分布图（2012年）.
Year WMAP image of the cosmic microwave background radiation(2012).因为发现宇宙微波背景辐射，彭齐亚斯和威尔逊获得了1978年度的诺贝尔物理学奖。
For discovering the Cosmic Microwave Background Radiation, Penzias and Wilson were awarded the 1978 Nobel Prize in Physics.世纪30年代，射电望远镜诞生，最终发现了脉冲星、类星体和宇宙微波背景辐射。
In the 1930s, the radio telescope was invented and eventually used to discover pulsars,quasars and the cosmic microwave background radiation.但所有上述运动速度都远低于天体自身相对于宇宙微波背景辐射（CMBR）的运行速度。
But these speeds are less than thespeed that all of theseobjects together move relative to the cosmic microwave background radiation(CMBR).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.而且，他们将利用正在或将要进行的欧洲空间局测量宇宙微波背景辐射和引力波的探测任务数据。
In particular, they will use data from current andfuture European Space Agency missions measuring cosmic microwave background radiation and gravitational waves.之后，1965年，彭齐亚斯（Penzias）和威尔逊（Wilson）偶然发现了宇宙微波背景辐射。
In 1965 Penzias and Wilson discovered the cosmic microwave background radiation.他和罗伯特·h·迪克等人一起预测了宇宙微波背景辐射。
With Robert Dicke and others, he predicted the cosmic microwave background radiation.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.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 然而，这些运动的速率都小于这些天体相对于宇宙微波背景辐射（CMBR）的运动速率。
But these speeds are less than thespeed that all of these objects together move relative to the cosmic microwave background radiation(CMBR).精确到几乎是宇宙微波背景辐射之前7次最佳单次实验结果的3倍”。
To a precision that is almost a factor of three better than 在普林斯顿，诺曼是专门测量宇宙微波背景辐射（CMBR）的重力集团的成员之一。
At Princeton,Norman is a member 宇宙微波背景辐射相关的研究，已经在1978年、2006年与2019年三次获得诺贝尔物理学奖。
The research on cosmic microwave background radiation has won the Nobel Prize in physics for three times in 1978, 2006 and 2019.此理论在1965年遭致命打击，宇宙微波背景辐射被发现。
This theory was discounted in 1965 with 的Q/U成像实验(安静)2008年10月开始观测宇宙微波背景辐射的极化。
此理论在1965年遭致命打击，宇宙微波背景辐射被发现。
The hypothesis was disproved by the 1965 discovery of cosmic microwave background radiation.两位名叫ArnoPenzias和RobertWilson的科学家正在研究这种现象，称为宇宙微波背景辐射（CMB）。
Two scientists named Arno Penzias and Robert Wilson were researching the phenomenon,known as Cosmic Microwave Background radiation(CMB).
