Примеры использования Cosmic microwave на Английском языке и их переводы на Русский язык
{-}
-
Official
-
Colloquial
The cosmic microwave background radiation… is the most distant thing we can see.
The faint glow of light collected by Planck is called cosmic microwave background radiation.
The discovery of the Cosmic Microwave Background(CMB) in 1964 confirmed a key prediction of the Big Bang cosmology.
The observatory site is also a temporary home to a cosmic microwave background observatory called AMiBA.
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.
His desk job involves poring through pages andpages of data about the cosmic microwave background.
The dipole anisotropy of the cosmic microwave background radiation was detected in 1969.
The pictures that emerged showed a special kind of radiation called the cosmic microwave background.
His work in black body form and anisotropy of the cosmic microwave background radiation cemented our understanding of the origin of the universe.
We see them in the picture of an afterglow from the Big Bang… andthey are known today… as the cosmic microwave background radiation.
Cosmic microwave background radiation was blisteringly hot when it was first created, but over the last 13 billion years, it has cooled dramatically.
Penzias and Wilson found evidence for the big bang theory with the concept of cosmic microwave background radiation.
POLARBEAR is a cosmic microwave background polarization experiment located in the Atacama Desert of northern Chile in the Antofagasta Region.
February 11- NASA's WMAP satellite completes the first detailed cosmic microwave background radiation map of the universe.
Inflation in the early universe, and the accelerated expansion of the universe has been confirmed by the recent observations of cosmic microwave radiation.
Research is taking place at Yerevan State University to examine the properties of cosmic microwave background radiation and to discover the large-scale structure and evolution of the early universe.
From its orbital position around the second Lagrangian point,Planck measures minute variations in the cosmic microwave background radiation.
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 cosmic structures.
A comoving observer is the only observer that will perceive the universe,including the cosmic microwave background radiation, to be isotropic.
It has made important confirmation of the Cosmic Microwave Background(CMB) anisotropy first measured by the Cosmic Background Explorer(COBE), launched in 1989, and it has begun to make a finer scale map of the CMB than is possible with the smaller antennas of COBE.
The total amount of baryonic dark matter can be inferred from models of Big Bang nucleosynthesis, and observations of the cosmic microwave background.
Two other effects which occurred between reionization and our observations of the cosmic microwave background, and which appear to cause anisotropies, are the Sunyaev-Zel'dovich effect, where a cloud of high-energy electrons scatters the radiation, transferring some of its energy to the CMB photons, andthe Sachs-Wolfe effect, which causes photons from the Cosmic Microwave Background to be gravitationally redshifted or blueshifted due to changing gravitational fields.
Simulations of this early galaxy formation matches the structure observed by galactic surveys as well as observation of the Cosmic Microwave Background.
At that time Jim Peebles pointed out,that in a Big Bang-created Universe there must have been a cosmic infrared background(CIB)- different from the cosmic microwave background- that can account for the formation and evolution of stars and galaxies.
The WCS standard includes many different spherical projections, including, for example,the HEALPix spherical projection widely used in observing the cosmic microwave background radiation.
The need for an accurate determination of the diffuse radio andmicrowave emission from the galactic disk was highlighted by the limitations imposed on cosmic microwave background data as a result of galactic foreground emission.
As we showed in the article,perception of superluminal motion also holds an explanation for cosmological phenomena like the expansion of the Universe and cosmic microwave background radiation.
Since the late 1980s or 1990s, most cosmologists favor the cold dark matter theory(specifically the modern Lambda-CDM model)as a description of how the universe went from a smooth initial state at early times(as shown by the cosmic microwave background radiation) to the lumpy distribution of galaxies and their clusters we see today-the large-scale structure of the universe.
Comme nous l'avons montré dans l'article,perception of superluminal motion also holds an explanation for cosmological phenomena like the expansion of the universe and cosmic microwave background radiation.
The need for an accurate determination ofthe diffuse radio and microwave emission from the galactic disk was highlighted by the limitations imposed on cosmic microwave background(CMB) data because of galactic foreground emission.