Examples of using Interferometer in English and their translations into Indonesian
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(3) we have compared it to previous interferometer results.
Like all interferometers, the instrument would split light and then recombine it to measure tiny changes, including motion.
Such device, called a Michelson interferometer.
They are called interferometers because they work by merging two or more sources of light to create an interference pattern, which can be measured and analyzed.
The latest research developments include the use of fibre optics,lasers and interferometers.
Interferometers are a type of instruments which work by superimposing two or more sources of light to create an interference pattern, which can be measured and analyzed.
Galaxy NGC5291(orange, at the center) and its ring of debris(in blue)as seen by the Very Large Array interferometer.
Lastly, September 14, 2015 LIGO Gravitational Wave Interferometer directly collecting and distortions in Spacetime resulted from the propagating ripple of the gravitational wave.
Because the path that one beam travels is a fixed length and the other is constantly changing as its mirror moves,the signal which exits the interferometer is the result of these two beams“interfering” with each other.
At last, on September 14, 2015,the LIGO Gravitational Wave Interferometer directly picked up the distortions in Spacetime resulting from the propagating ripples of gravitational waves.
For very high data rates or very long distance links, a laser source may be operated continuous wave, and the light modulated by an external device such as an electro-absorption modulator or Mach-Zehnder interferometer.
The name refers to theCombined Array for Research in Millimeter Astronomy(CARMA), an interferometer that was located in California, and the Nobeyama Radio Observatory(NRO) telescope, in Japan.
For conceiving and designing the Laser Interferometer Gravitational-Wave Observatory(LIGO), whose recent direct detection of gravitational waves opens a new window in astronomy, with the first remarkable discovery being the merger of a pair of stellar mass black holes.
Gratings, optical components which look like bunches of upright parallel bars,create interference in the X-ray beam, like an interferometer, merging sources of light to create an interference pattern that can be measured.
Other gravitational wave detectors- such as the Virgo interferometer near Pisa, Italy, and the GEO600 interferometer near Hannover, were not operating at the time of LIGO's observation and theerfore could not confirm the signal.
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The Westerbork Synthesis Radio Telescope(WSRT)is an aperture synthesis interferometer near World War II Nazi detention and transit camp Westerbork, north of the village of Westerbork, Midden-Drenthe, in the northeastern Netherlands.
As of 2013, operational facilities located at the Hanford Site included: The Pacific Northwest National Laboratory, owned by the Department of Energy and operated by Battelle Memorial Institute The Fast Flux Test Facility(FFTF), a national research facility in operation from 1980 to 1992 whose last fuel wasremoved in 2008 LIGO's Hanford Observatory, an interferometer searching for gravitational waves Columbia Generating Station, a commercial nuclear power plant operated by Energy Northwest.
Such an experiment could be carried out by the Laser Interferometer Gravitational-Wave Observatory(LIGO) in the US, whose twin detectors, 2000 miles apart, directly detected gravitational waves for the first time in 2015.
Other noteworthy telescopes operated at Cal-Tech include a telescope to search for supernovae, a comet hunter, a trio of sky cameras looking for planetary andother celestial phenomena, an interferometer capable of detecting the slightest wobble in the orbits of a planet, and a sixty inch telescope responsible for spotting the first brown dwarf circling a companion star.
Two experiments- the Laser Interferometer Gravitational-Wave Observatory in the United States and Virgo in Italy- have now been able to measure changes in the dimensions of space-time of a fraction of the diameter of a proton, caused by waves created in the collisions of black holes or neutron stars.
The gravitational waves they emit cause ripples inspace-time that can be detected by the Laser Interferometer Gravitational-Wave Observatory(LIGO) and the Virgo experiments, giving a precise measurement of the system's distance from Earth.
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The device built by Tanzilli's group functions similarly- the interferometer is closed for vertically polarized photons(which therefore act as waves) and open for horizontally polarized photons(which behave as particles).
The team hasshown that all it takes is a beam of neutrons and an interferometer- a detector that measures interference patterns- to create direct visual representations of an object and reveal details about specific points within it.
All three scientists have played leading roles in the Laser Interferometer Gravitational-Wave Observatory, or Ligo, experiment, which in 2015 made the first historic observation of gravitational waves triggered by the violent merger of two black holes a billion light-years away.
The announcement in February that scientists from the Laser Interferometer Gravitational-Wave Observatory(LIGO) unlocked the final door to Albert Einstein's Theory of Relativity- proof that gravitational waves produce ripples through space and time- has a rich back-story involving HTCondor.