「interferometers」の共起表現(1語右で並び替え)

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「interferometers」の共起表現一覧(1語右で並び替え)

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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

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「interferometers」の共起表現一覧(1語右で並び替え)