Examples of using Interferometer in English and their translations into Danish
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Yeah, using an interferometer to create what is… Right.
ESO has been a pioneer in this field with the Very Large Telescope Interferometer(VLTI) at Paranal.
Set up a Michelson interferometer, and understand basic aspects of interference.
These can be combined with the Unit Telescopes to make the Very Large Telescope Interferometer VLTI.
Use an advanced semiconductor-based interferometer as an optical switch.
This beauty has an interferometer, which can convert the readings back into crystal-clear sound.
Juan Pablo Henríquez, a mechanical technician,adjusting the delay lines of the VLTI Very Large Telescope Interferometer.
Set up a Fabry-Perot interferometer, and use it for spectral resolution of laser modes.
The VLT also offers the possibility to combine the light from the four UTs to work as an interferometer.
The VLT Interferometer(VLTI) can also make use of four 1.8-metre Auxiliary Telescopes(ATs) that can be moved along the platform to get more information about the object.
Credit: ESO Juan Pablo Henríquez, a mechanical technician,adjusting the delay lines of the VLTI Very Large Telescope Interferometer.
The Very Large Telescope Interferometer(VLTI), with its own suite of instruments, ultimately providing imagery at the milliarcsecond level as well as astrometry at 10 microarcsecond precision.
One of the most exciting features of the VLT is the option to use it as a giant optical interferometer VLT Interferometer or VLTI.
An interferometer combines the light from two or more telescopes, allowing astronomers to pick out the details of an object as though they are being observed using mirrors or antennas measuring hundreds of metres in diameter.
I propose that this cosmic gravitational background radiation should be looked for by the projected LIGO detector Laser Interferometer Gravitational-wave Observatory!
The telescopes can work together,to form a giant'interferometer', the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes.
ALMA is composed of 66 high precision antennas, operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, each measuring 12 metres in diameter,acting together as a single telescope- an interferometer.
To visit the ALMA Site,please see Media Visits Why is ALMA an interferometer? ALMA is a single telescope of revolutionary design, composed initially of 66 high-precision antennas, and operating at wavelengths of 0.32 to 3.6 mm.
The partnership between ESO and the CTAO will serve as the cornerstone in the fast-growing era of multi-messenger astrophysics, providing an opportunity for further collaboration with other large infrastructures, such as the Atacama Large Millimeter/submillimeter Array(ALMA),the Square Kilometre Array(SKA) and state-of-the-art gravitational-wave interferometers.
It was first studied andclassified a few years ago by researchers using ESO's Very Large Telescope Interferometer(VLTI) when it was found to be something known as a yellow hypergiant, a massive and luminous type of star that is extremely rare- and extremely big!
Now, the use of highly sophisticated interferometers like ALMA, coupled with a dose of mathematics, mean that astronomers can produce a picture almost as detailed as the one obtained with a full-size mirror hundreds of metres in diameter or a giant antenna several kilometres wide.
The event will be observable by the GRAVITY instrument on the Very Large Telescope Interferometer(VLTI), Atacama Large Millimeter/submillimeter Array(ALMA), and the forthcoming European-Extremely Large Telescope(E-ELT), providing a good chance of ascertaining the mass of any planet to a high degree of accuracy.
