This idea is embodied in the Fermi Paradox.
这个想法在费米悖论中有所体现。
But over the next few years, Fermi will detect more and more bursts.
不过随着时间的推移，费米望远镜会不断发现更多的爆发点。
So Enrico Fermi called them "a little neutron," in Italian is neutrino.
因此，恩里科·费米把它们叫做‘小中子’，在意大利语中就是中微子的意思。
He believes that this process supplies the gamma-rays observed by Fermi.
他相信这个过程产生出了费米镜观测到的伽马射线流。
On September 16, 2008, Fermi picked up the most powerful GRB observed to date.
2008年9月16日，费米望远镜发现了迄今为止最为强烈的伽马射线爆发。
At these temperatures, the gas takes on a very exotic form; it becomes a Fermi gas.
在这个温度下，气体处于一种奇异的形态：它成为了费米气体。
The Fermi bubbles could be powered by the black hole at the center of our galaxy.
费米尔泡可能是由我们银河系中心的黑洞所驱动的。
PSR J0357 was originally discovered by the Fermi Gamma Ray Space Telescope in 2009.
PS r J 0357最初是通过费米·伽玛射线太空望远镜(Fermi Gamma Ray Space Telescope)于2009年发现的。
Jim Fermi is allowed to enter his office in the Engineering Building; Private office 2.
允许Jim Fermi进入工程楼中他自己的办公室，即个人办公室2。
Jim Fermi is allowed to enter his office in the Engineering Building, Private office 2.
允许Jim Fermi进入工程楼中他自己的办公室，即个人办公室2。
Researchers called them Fermi bubbles, after the Fermi space telescope that spotted them.
鉴于费米尔望远镜发现了它们，研究人员称其为费米尔泡。
Grant Jim Fermi the privilege to lock the lab anytime he wants so that he can work undisturbed.
授予JimFermi在任何时间锁住实验室门的权限，以便他能在不受打扰的情况下工作。
This speaks to the Fermi Paradox, which asks why the galaxy isn't crawling with intelligent life.
这是回答费米悖论所提问的，为什么星系中没有充满了智能生命。
In superconductors, the bosons are the pairs of bound electrons that form at the Fermi surface.
在超导体中，玻色子是在费密表面形成的束缚态电子对。
In fact, the September 16th burst is the most powerful observed to date, and was easily detected by Fermi.
事实上，9月16日观测到的爆发是迄今为止最为强烈的，所以费米望远镜很容易就发现了它。
This morning we noticed that one of the many active galaxies in the Fermi sky had become extremely bright in gamma-rays.
早上，我们从费米伽马射线图中的众多活跃星系中观察到，其中一个星系的伽马射线变得极度明亮。
More observations from Fermi, while useful in clarifying the bubbles' exact shape, probably won't resolve how they formed.
如果有更多的费米望远镜观测结果，将会有助于弄清楚气泡结构的准确形状，但恐怕将不会有助于搞清楚它形成的原因。
Soon after launch, Fermi started picking up gamma-ray bursts (GRBs), powerful explosions usually triggered by dying stars.
发射成功后不久，费米太空望远镜即开始收集伽马射线爆发(GRBs)的迹象，通常这种强烈的爆发是由濒死的恒星造成的。
In Table 3, for example, Jim Fermi is configured to enter a variety of rooms and LABS, but is not configured to enter the campus.
例如，在表3中，JimFermi配置为可以进入多个房间和实验室，但是未配置为可以进入校园。
Studying such atomic waves has led to the discovery of new states of matter—Bose-Einstein condensates and degenerate Fermi gases.
超冷原子的德布罗意波波长的研究导致了新的发现比如波色-爱因斯坦凝聚状态和气体的简并压力。
Lots of galaxies exhibit two-lobed jets of matter and energy erupting from their cores, but the "Fermi bubbles" defy easy explanation.
许多星系都呈现出双泡状物质喷流并且伴有核心区域喷发出的能量，不过“费米气泡”已然超越了这种简单的解释。
Two 30,000 light-year-long blobs called Fermi bubbles have been discovered on either side of our galactic plane. John Matson reports
在银河盘面两端，发现了两个长达30,000光年的东东，它们被称作费米尔泡。
It should be relatively straightforward to detect these using satellite-based telescopes such as Fermi, which was launched last year.
这应该能相对直接地用太空望远镜探测到，例如去年发射的费尔米太空望远镜。
Fermi was located immediately above a thunderstorm for most of the observed gamma-ray flashes, but in several cases, storms were far away.
把费米直接去监察一次雷暴雨，以便能观察到大多数的伽玛射线闪光，但在有些情况下，风暴已远远地离去。
The Fermi Space Telescope found hints in 2009 of the telltale pattern associated with positrons in terrestrial gamma rays stemming from lightning storms.
费米太空望远镜在2009年就曾发现这一与正电子有关的特征现象的线索，地点正是在源于雷暴的地表伽马射线中。
The Fermi Space Telescope is so sensitive to these gamma ray bursts that it doesn't even need to be positioned right over a thunderstorm to detect the TGFs.
费米太空望远镜对这些伽马射线脉冲很灵敏，以至于它甚至不需要调整位置对准雷暴的正上方，就能来探测TGF信号。
The Fermi Space Telescope is so sensitive to these gamma ray bursts that it doesn't even need to be positioned right over a thunderstorm to detect the TGFs.
费米太空望远镜对这些伽马射线脉冲很灵敏，以至于它甚至不需要调整位置对准雷暴的正上方，就能来探测TGF信号。
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