However, it's one of the best spots on the planet for surveying
the faint cosmic microwave background (CMB) radiation left over from the Big Bang.
Not exact matches
[6]
Cosmic - infrared background radiation, similar to the more famous cosmic microwave background, is a faint glow in the infrared part of the spectrum that appears to come from all directions in
Cosmic - infrared
background radiation, similar to the more famous
cosmic microwave background, is a faint glow in the infrared part of the spectrum that appears to come from all directions in
cosmic microwave background, is a
faint glow in the infrared part of the spectrum that appears to come from all directions in space.
That ancient, relic light washes over us even now, diminished by the intervening eons to a
faint all - sky
microwave glow: the
cosmic microwave background (CMB).
Along with the familiar
cosmic microwave background — the afterglow of the big bang — the distant universe is suffused with an infrared
background, thought to come from galaxies and stars too
faint and far away to see.
These primordial gravitational waves are too
faint to be detectable directly, but it should be possible to see their imprint on the relic radiation from the big bang — the
cosmic microwave background.
Gravitational waves from inflation generate a
faint but distinctive twisting pattern in the polarization of the
cosmic microwave background, known as a «curl» or B - mode pattern.
These groundbreaking results came from observations by the BICEP2 telescope of the
cosmic microwave background — a
faint glow left over from the Big Bang.
The
Cosmic Microwave Background radiation, or CMB for short, is a
faint glow of light that fills the universe, falling on Earth from every direction with nearly uniform intensity.
The telescope has helped researchers detect such clusters by exploiting a phenomenon known as the Sunyaev - Zel «dovich effect, which causes massive galaxy clusters to leave an impression on the
cosmic microwave background: a
faint, universe - spanning glow of light left over from the big bang.
The
cosmic microwave background is a
faint glow that pervades the entire sky, dating back to just 380,000 years after the big bang.
Working with a tough mentor named Yakov Zel «dovich, Sunyaev showed that the tiny acoustic vibrations in the universe moments after the Big Bang could be observed as temperature and density variations in the
cosmic microwave background (CMB) radiation, the
faint afterglow of the Big Bang that suffuses the universe.
Lee Smolin of the Perimeter Institute for Theoretical Physics noted that some forms of quantum gravity predict certain asymmetries — one direction of polarization might be favored over another — that could be imprinted in the
cosmic microwave background (CMB), a
faint echo of radiation from the early universe.
Previously, the most precise test of cosmological models came from measurements with the European Space Agency's Planck satellite of what is known as the
cosmic microwave background (CMB)-- a
faint glow in the sky emitted 380,000 years after the Big Bang.
The researchers used radio telescopes at the South Pole to stare at the
cosmic microwave background radiation — a
faint afterglow left over from the big bang that permeates the universe.
The extremely dry, cold air is perfectly suited for observing
Cosmic Microwave Background (CMB) radiation - the
faint light signature left by the Big Bang that brought the universe into being nearly 14 billion years ago.