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- Interferometry - Wikipedia
Interferometry typically uses electromagnetic waves and is an important investigative technique in the fields of astronomy, fiber optics, engineering metrology, optical metrology, oceanography, seismology, spectroscopy (and its applications to chemistry), quantum mechanics, nuclear and particle physics, plasma physics, biomolecular interactions
- Basics of Interferometry - Georgia State University
Basics of Interferometry The resolution of a telescope is set by the size of its primary mirror or lens The larger the diameter of the telescope, the higher the spatial resolution, improving its ability to see finer details
- What is an Interferometer? | LIGO Lab | Caltech
A description of an interferometer, a diagram Because of their wide application, interferometers are used to measure everything from the smallest variations on the surface of a microscopic organism, to the structure of enormous expanses of gas and dust in the distant Universe, and now to detect the nearly imperceptable motions caused by gravitational waves (a distance 1 1,000 th the width of
- How do interferometers work? - Explain that Stuff
The basic idea of interferometry involves taking a beam of light (or another type of electromagnetic radiation) and splitting it into two equal halves using what's called a beam-splitter (also called a half-transparent mirror or half-mirror)
- Interferometry explained - Renishaw
'Interferometry' is a measurement method using the phenomenon of interference of waves (usually light, radio or sound waves) The measurements may include those of certain characteristics of the waves themselves and the materials that the waves interact with
- Interferometry Explained - National Radio Astronomy Observatory
With interferometry, radio astronomers can combine the signals from many antennas, and even many telescopes It allows them to create an image that is much brighter and sharper than what is possible from a single antenna dish
- Basics of Optical Interferometry: A Gentle Introduction
1 Introduction: Interferometry is Inevitable Stars are, from an angular size standpoint, small This rather qualitative, relative statement can actually be easily quantified in a back-of-the-envelope fashion Using our sun – an object of 30 minutes of arc in angular diameter† – as a prototype, we can rapidly
- How Interferometry Works, and Why its so Powerful for Astronomy
From the inauguration of the VLA in 1980 to the first light of ALMA in 2013, interferometry has given us extraordinarily high-resolution images The technique is now so powerful that it can be
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