普勒 - 翻译成英语

kepler
开普勒
克卜勒
开普勒太空望远镜
自开普勒
doppler
多普勒
都卜勒
多普勒仪
puller
普勒

在 中文 中使用 普勒 的示例及其翻译为 英语

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几年前,当开普勒太空望远镜遭遇严重故障时,许多人确信它的任务已经结束。
When the Kepler space telescope suffered its critical malfunction a few years ago, many people were convinced that its mission had ended.
在当前和更先进的彩色多普勒成像(CDI)的彩色编码脉冲多普勒信息是基于B型超声图像叠加。
In the current and more sophisticated color Doppler imaging(CDI), color-coded pulsed Doppler information is superimposed on a B-mode ultrasonic image.
例如,用开普勒太空望远镜完成的系外行星的观测显示太阳系与我们自己的系统不同。
Observations of exoplanets done with the Kepler Space Telescope, for example, have revealed solar systems wildly unlike our own.
为了理解这种现象的含义,我们必须首先了解多普勒效应。
To understand the implications of this, we must first understand the Doppler effect.
美国国家航空航天局开普勒太空望远镜可能不再做什么了,但由于它留下的数据,这些发现仍在进行中。
NASA's Kepler Space Telescope might not be doing much anymore, but discoveries are still being made thanks to the data it left behind.
经过多年的努力,精心研制出了“超声多普勒血流检测仪“。
After years of efforts, carefully developed the"ultrasonic doppler blood flow detector.".
此前,机器学习的方式已经被用于筛选、分类普勒的数据,但是,Shallue的神经网络能够提供更加强大的算法。
Machine-learning approaches have been used to filter and classify Kepler data before, but Shallue's neural network offered a far more powerful algorithm.
该频率与FMCW雷达的载波频率遵守相同的规律(如多普勒效应)。
This frequency is subject to the same laws(e.g. Doppler effect) as the carrier frequency in FMCW radar.
这项开普勒太空望远镜的最新使命帮助天文学家采集了最完整的昂宿星团恒星自转速度。
The latest mission by the Kepler space telescope has helped astronomers collect the most complete catalog of spin rates among the stars of the Pleiades cluster.
他表现出超声波脉冲多普勒测距选通,并且是恶性肿瘤新血管形成的超声多普勒信号特性的发现者。
He demonstrated ultrasonic pulsed-Doppler range-gating, and was the discoverer of the ultrasonic Doppler signal characteristic of malignant tumour neovascularisation.
然而到1624年,紧张关系的升级以及预言的不准确意味着给开普勒自身带来的政治麻烦;.
By 1624, however, the escalation of those tensions and the ambiguity of the prophecies meant political trouble for Kepler himself;
这为天文学家提供了一种发现行星的新方法,那就是利用多普勒效应。
And that gives astronomers a way to find them, using the Doppler effect.
最终,TESS将探测90%的天空,它的探测范围将比开普勒太空望远镜大400倍。
As a result, TESS will detect 90% of the sky and will be able to detect 400 times more than the Kepler Space Telescope.
用我们的工作模型,我们拍摄了恒星,用它来寻找开普勒数据中的新行星。
Armed with our working model, we shot for the stars, using it to hunt for new planets in Kepler data.
在个人写给开普勒在1598年,伽利略指出,他是一个哥白尼(相信哥白尼的理论)。
In a personal letter written to Kepler in 1598, Galileo had stated that he was a Copernican(believer in the theories of Copernicus).
这一宣布使开普勒证实的行星数目增加了一倍以上。
The announcement more than doubled the number of confirmed planets from Kepler in one sweep.
但这并不能解释开普勒观测到的一个令人困惑的问题:相当于地球半径1.5倍到两倍之间的行星非常少。
But that can't explain a puzzling gap observed by Kepler: There are very few planets with sizes between 1.5 and 2 Earth radii.
齐伯斯坦很好奇,想知道开普勒的论文中是否会出现类似的金属。
Zilberstein was curious to see if similar metals would turn up in Kepler's papers.
为了这批新发现,科学家们从开普勒发回的大量数据中进行了筛选。
For these new discoveries, scientists screened a large amount of data back from Kepler.
月26日,科学家宣布从开普勒数据中,证实了715颗新的系外行星。
On February 26, scientists announced that data from Kepler had confirmed the existence of 715 new exoplanets.
结果: 108, 时间: 0.0379

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