etalon

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(redirected from Fabry-Perot Interferometer)

e·ta·lon

 (ā′tə-lŏn′, ĕt′ə-)
n.
A type of interferometer in which incoming light is repeatedly refracted and reflected between two surfaces into multiple beams that are then focused together, causing self-interference of the light.

[French étalon, standard (of weight or a unit of measurement), reference point, etalon (in reference to the fixed widths between the two surfaces in the first such interferometers), from Old French estalon, standard, of Germanic origin; akin to Middle Dutch stael, model, sample.]
American Heritage® Dictionary of the English Language, Fifth Edition. Copyright © 2016 by Houghton Mifflin Harcourt Publishing Company. Published by Houghton Mifflin Harcourt Publishing Company. All rights reserved.

etalon

(ˈɛtəˌlɒn)
n
(General Physics) physics a device used in spectroscopy to measure wavelengths by interference effects produced by multiple reflections between parallel half-silvered glass or quartz plates
[C20: French étalon a fixed standard of weights and measures, from Old French estalon; see also stallion]
Collins English Dictionary – Complete and Unabridged, 12th Edition 2014 © HarperCollins Publishers 1991, 1994, 1998, 2000, 2003, 2006, 2007, 2009, 2011, 2014
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References in periodicals archive
Ahmad, "Chronology of Fabry-Perot interferometer fiber-optic sensors and their applications: a review," Sensors, vol.
2 PRINCIPLE AND STRUCTURE OF THE SENSOR 2.1 Principle of the Fabry-Perot interferometer
Kim, "Measuring dynamic strain of structures using a gold-deposited extrinsic Fabry-Perot interferometer," Smart Materials and Structures, vol.
Huang, "Extrinsic fiber-optic Fabry-Perot interferometer sensor for refractive index measurement of optical glass," Applied Optics, Vol.
Monchalin, Optical detection of ultrasound at a distance using a confocal Fabry-Perot interferometer, Appl.
This system also has a long-pulse high-power neodymium-YAG laser (featuring high-frequency and amplitude stability) for detection and a confocal Fabry-Perot interferometer for measuring the resulting surface vibrations.
Fabry-Perot interferometer based optical spectrum analyzers have a narrow resolution, typically specified in frequency between 100 MHz and 10 GHz.
The astronomers embarked on their odyssey using a special instrument, a Fabry-Perot interferometer. Acting like a highly selective filter, it uses the wave-like properties of light and a variable gap between two polished mirrors to pick out whatever visible-light wavelength the astronomers choose to view.
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