cosmic microwave background造句1. This cosmic microwave background radiation, they said, represents the ancient afterglow of the big bang.
2. Fluctuations in the cosmic microwave background radiation probe the earliest moments of the universe.
3. However, measurements of the cosmic microwave background radiation temperature suggest that its structure may have some systematic order.
4. These gases scatter light from the cosmic microwave background radiation as it passes through the clusters, similar to the way Earth's atmosphere can scatter starlight, making some stars twinkle.
5. And Wilson and Penzias discovered the cosmic microwave background radiation, physical evidence for the Big Bang, while fiddling with an antenna designed to catch radio waves bouncing off satellites.
6. The glow of cosmic microwave background radiation, which is found throughout the universe, is thought to be a tangible remnant of leftover light from the big bang.
7. The mottled look of the Cosmic Microwave Background radiation is the result of differences in temperature and density.
8. This is the famous cosmic microwave background (CMB) radiation, and a key target of the Planck mission.
9. Model of the power spectrum of the cosmic microwave background radiation ( CMBR ) by Prof M.
10. Image of the cosmic microwave background radiation ( CMBR ).
11. This echo is known as cosmic microwave background (CMB) radiation, a remnant of the vast energies unleashed as the universe burst into being.
12. The South Pole Telescope, which began scientific observations in 2007, surveys the sky for cosmic microwave background radiation, the "afterglow" of the Big Bang.
13. Much of the progress has come through studies of the afterglow of the big bang, radiation known as the cosmic microwave background (CMB).
14. You might say , well, look, we have the cosmic microwave background radiation.
15. Kashlinsky and colleagues first noticed the dark flow when studying the way gas in galaxy clusters interacts with the cosmic microwave background radiation.
16. They had found the cool afterglow of the big bang: the cosmic microwave background radiation.
17. Data from the Wilkinson Microwave Anisotropy Probe (WMAP) can show the minute temperature changes created as the cosmic microwave background radiation moves through gases in galaxy clusters.
18. Cosmologists usually consider the dust-emitted microwaves to be “noise” that obscures their data, worth analyzing only to erase from their measurements of the cosmic microwave background.
19. Brighter clusters—those with more hot gases—would be expected to have greater affects on the cosmic microwave background, and that's what the new study confirmed.
20. His work in black body form and anisotropy of the cosmic microwave background radiation CEMENTED our understanding of the origin of the universe.
21. If two universes had collided, the researchers say, it would have left a circular pattern behind in the cosmic microwave background.
22. Developed and built at Goddard Space Flight Center in Greenbelt, Md., COBE precisely measured and mapped the oldest light in the universe -- the cosmic microwave background.
23. Such collisions would have left lasting marks in the cosmic microwave background (CMB) radiation, the diffuse light left over from the Big Bang that pervades the universe, the researchers say.
24. The recent progress on observation and theory of the cosmic microwave background radiation(CBR) is presented in this paper.
25. If multiple universes exist, they may collide with each other and leave behind signs in the cosmic microwave background radiation, researchers say.
26. Many of the recent studies in cosmology focus on the cosmic microwave background (CMB).
27. The nature of this system is completely different from the one of an equilibrium state of photons, which is just the cosmic microwave background radiation observed.
28. A universe shaped like a Bugle may sound odd, but it could help explain some puzzling observations of the cosmic microwave background radiation: the relic radiation left over from the big bang.
29. WMAP was designed to provide a more detailed look at subtle temperature differences in the cosmic microwave background that were first detected in 1992 by NASA's Cosmic Background Explorer (COBE).
30. The presence of dark energy has been independently backed up by measurements of the cosmic microwave background, the radiation left over from the big bang.