Примери за използване на Cosmic microwave на Английски и техните преводи на Български
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Cosmic Microwave Background.
However, if the cosmic microwave radiation….
The cosmic microwave background is a barrier that blocks our vision.
A dark bruise, superimposed on the cosmic microwave background.
The cosmic microwave background.
In 1965 there was opened cosmic microwave radiation.
The cosmic microwave background.
This first light is called the Cosmic Microwave Background.
In 1965 cosmic microwave background radiation was discovered.
This is the origin of the CMB: the Cosmic Microwave Background.
In 1965, the Cosmic Microwave Background Radiation was detected.
The horizon problem correlates with the cosmic microwave background issue.
The discovery of the cosmic microwave background opened a window into the origins of the universe.
His desk job involves poring through pages andpages of data about the cosmic microwave background.
The Cosmic Microwave Background as measured by the Wilkinson Microwave Anisotropy Probe(WMAP).
In particular, they used the light from the cosmic microwave background, or CMB for short.
The cosmic microwave background radiation is one such place, and the distribution of galaxies is another.
Gravitational waves stretching and compressing would leave an effect on the polarisation of the cosmic microwave background.
The discovery of the cosmic microwave background, and observations of black holes, support these conclusions.
This is confirmed by observations of small non uniformities in the cosmic microwave background, with exactly the predicted properties.
It's called the cosmic microwave background, and it's a picture of the way the Universe looked about 400,000 years after the Big Bang.
These guys point out that any object traveling at relativistic speeds will interact with photons in the cosmic microwave background.
This is what we now see as the cosmic microwave background- the glow of light from a time when the universe could finally be seen.
Astronomers have even estimated its value based on observations of distant supernovas and fluctuations in the cosmic microwave background.
This cosmic microwave background, this CMB, as we call it, we think of as the afterglow of the heat of the big-bang explosion itself.
And those fluctuations were stretched to astronomical sizes, andthose fluctuations eventually are the things we see in the cosmic microwave background.
This picture shows the cosmic microwave background radiation measured by the European Space Agency‘s Planck satellite observatory.
The researchers posited that the earliest stars likely changed the universe's background electromagnetic radiation,also known as cosmic microwave background(CMB).
But if the Cosmic Microwave Background group is mistaken, and the expansion rate is closer to 73 km/s/Mpc, it foretells a crisis in modern cosmology.
The best evidence for dark matter today comes from measurements of something called the cosmic microwave background, the afterglow of the Big Bang, but that's another story.