interferometry's Usage Examples:

Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy.

astronomical objects such as stars, nebulas and galaxies by means of interferometry.

Dual-polarization interferometry (DPI) is an analytical technique that probes molecular layers adsorbed to the surface of a waveguide using the evanescent.

In contrast, interferometry uses differential phase of the reflected radiation, either from multiple.

telescopes utilizing the techniques of radio interferometry and aperture synthesis.

The use of interferometry allows radio astronomy to achieve high angular.

Aperture synthesis or synthesis imaging is a type of interferometry that mixes signals from a collection of telescopes to produce images having the same.

divided into the shift-and-add ("image stacking") method and the speckle interferometry methods.

It aims to measure gravitational waves directly by using laser interferometry.

Volcano and earthquake monitoring use differential interferometry.

amplitude interferometry is used for the determination of lengths, surface irregularities and indexes of refraction; intensity interferometry, besides.

Optical coherence tomography is based on low-coherence interferometry, typically employing near-infrared light.

resolution observations of cosmic radio sources using very-long-baseline interferometry (VLBI).

after French physicist Georges Sagnac, is a phenomenon encountered in interferometry that is elicited by rotation.