Examples of using Interferometer in English and their translations into German
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News from the interferometer MAX+: New compact design.
A mirror sends some of the light back towards the laser,which directs it again towards the interferometer.
White-light interferometer for integrated quality control.
Measuring of surface flatness with a Zygo GPI interferometer λ/10 accuracy.
In addition to all common mounts for your interferometer, we also deliver comprehensive solutions for the alignment of CGHs and test objects.
People also translate
A mirror returns all the unused light back towards the laser,which directs it again towards the interferometer.
The AN/APG-78 and radar frequency interferometer are housed in a dome located above the main rotor.
They are currently developing the most powerful interferometric instrument in the world,the VLTI Very Large Telescope Interferometer.
The pending request to use the Foundation's sensitive interferometer on research with 298 has been denied.
As measuring system for position control, PI uses an internally developed optical linearencoder that is based on an integrated Mach-Zehnder interferometer.
Bruker's VERTEX 70v FTIRSpectrometer is based on the well-known RockSolid™ interferometer and the ideal entry level systems for Advanced Research applications.
During the interferometric inspection of optical surfaces,an exact alignment of the lens elements with respect to the interferometer is necessary.
In this case the interferometer mirror moves very fast and up to 4 spectra can be extracted from each full forward-backward interferometer scan.
Some of these characteristics, such as, for example, the polishing radius, apex offset, or fiber protrusion,can be measured with an interferometer; however, the concentricity cannot be measured.
The innovative and award-winning Tilted Wave Interferometer MarOpto TWI 60 checks the entire surfaces of polished aspheres, automatically, without contact and within seconds without stitching or CGH.
Future detectors are being developed or planned, which will greatly improve the sensitivity of these experiments, suchas the Advanced LIGO detector due to start operation in 2015, and the proposed evolved Laser Interferometer Space Antenna eLISA.
But this star is quite distant and the full power of the Very Large Telescope Interferometer(VLTI) was needed to resolve very fine details and see what is going on in the dust disc.”.
And in 2034, the eLISA interferometer is to listen from space for low-frequency gravitational waves from the whole visible universe and thus supplement the ground-based detectors.
But this star is quite distant andthe full power of the Very Large Telescope Interferometer(VLTI) was needed to resolve very fine details and see what is going on in the dust disc.
An interferometer takes a beam of light and splits it, then recombines it, and from the interference pattern produced we can measure how much further one beam travelled than the other see interferometer section.
If the spectrum of measurable parts has expanded towards larger parts,it is possible to retrofit the TOPOS 100 interferometer with a cross or rotary table and hence, adapt the instrument towards the new measurement requirements.
The heart of the MultiRAM is Bruker's patented interferometer with gold coated optics and permanent RockSolidTM alignment, which provides the superb stability and throughput required for demanding emission experiments, as it is the case for Raman spectroscopy.
Inconceivable, but true: if you want to detect gravitational waves, you must measure the mutual shift of two light waves by a hundred billionth of a degree(10-11)-a"nothing" which an interferometer converts into a tiny difference in brightness.
Using high sensitivity newly refurbished detectors for radio waves in themillimeter range at the Plateau de Bure Interferometer,* the authors of this here presented work have been able for the first time to measure the molecular gas content of ordinary and representative galaxies in the distant Universe.
MATISSE, the Multi-AperTure mid-Infrared SpectroScopic Experiment, has passed a suite of initial tests conducted at the Observatoire de la Côte d'Azur in France andwill now be transported to Chile for integration into the Very Large Telescope Interferometer(VLTI) at ESO's Paranal Observatory.
Due to its very high resolution of high-frequent errors and extremely short measuring times,the Tilted Wave Interferometer is particularly suited for the quality assurance of modern optics as a measuring system in the production process.
In order to investigate the immediate environment of a young star with unprecedented accuracy, an international team of researchers led by Fabien Malbet of the University of Grenobleused two telescopes of the Very Large Telescope Interferometer(VLTI) of the European Southern Observatory(ESO), which is located on the Cerro Paranal mountain in Chile.
On 14 September 2015, 5:51 on the USEast Coast, the LIGO detectors- Laser Interferometer Gravitational Wave Observatory, in Livingston, Louisiana, and Hanford, Washington state, measured the waves caused in the space-time continuum, gravitational waves, which reached Earth from a cataclysmic event that happened somewhere far in the Universe.
Data repositories provide access to a climatology of polar stratospheric clouds(PSC)and general cloud information obtained from the Michelson Interferometer for Passive Atmospheric Sounding(MIPAS) instrument onboard the Envisat satellite ESA.