「interferometers」の共起表現(1語右で並び替え)

A overview of Astronomical interferometers and a History of astronomical interferome

niques can be considered theoretically as interferometers and, as such, their ultimate sensitivitie

Fizeau interferometers are often used to do this.

Interferometers are typically used to accurately measure

Lummer-Gehrcke interferometers are now rarely used, having been largely

Michelson interferometer and Mach-Zehnder interferometers are examples of such systems.

These interferometers are useful in optical metrology and have

N-slit interferometers are also of interest to researchers worki

telescope types and List of astronomical interferometers at visible and infrared wavelengths.

meter is one of the earliest astronomical interferometers built and used.

ers or Fourier Transform Infrared (FT-IR) interferometers, depending on the application.

igh precision experiments now employ atom interferometers due to their short de Broglie wavelength.

Such interferometers had a wide range of applications, for exa

are reversed compared to the laser based interferometers, i.e. the beam splitter and mirrors are l

he frequency of a laser (connected to all interferometers in the system) and counting fringe cycles

elation of signals from several different interferometers located around the Sun.

At radio wavelengths, interferometers such as the Very Large Array and MERLIN h

Early interferometers used white light sources and also monochr

This approach was extended to N-slit interferometers using narrow-linewidth laser illumination

m were diagramming ground-based, tracking interferometers, which relieved the Viking of the burden

most sensitive polarimeters are based on interferometers, while more conventional polarimeters are

「interferometers」の共起表現一覧(1語右で並び替え)