Gires-Tournois interferometer - meaning and definition. What is Gires-Tournois interferometer
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What (who) is Gires-Tournois interferometer - definition

Gires-Tournois interferometer; Gires-Tournois etalon; Gires–Tournois interferometer

GiresTournois etalon         
In optics, a GiresTournois etalon is a transparent plate with two reflecting surfaces, one of which has very high reflectivity, ideally unity. Due to multiple-beam interference, light incident on a GiresTournois etalon is (almost) completely reflected, but has an effective phase shift that depends strongly on the wavelength of the light.
Twyman–Green interferometer         
SCIENTIFIC INSTRUMENT
Twyman-green interferometer; Twyman-Green Interferometer; Twyman-Green interferometer
A Twyman–Green interferometer is a variant of the Michelson interferometer principally used to test optical components. It was introduced in 1916 by Frank Twyman and Arthur Green.
Livre tournois         
CURRENCY
Livre Tournois; Livres; Tournai pound; French livre tournois; Livres tournois; ₶; Sols tournois; Tours pound; Sous tournois
The (; ; abbeviation: ₶.) was one of numerous currencies used in medieval France, and a unit of account (i.

Wikipedia

Gires–Tournois etalon

In optics, a Gires–Tournois etalon is a transparent plate with two reflecting surfaces, one of which has very high reflectivity, ideally unity. Due to multiple-beam interference, light incident on a Gires–Tournois etalon is (almost) completely reflected, but has an effective phase shift that depends strongly on the wavelength of the light.

The complex amplitude reflectivity of a Gires–Tournois etalon is given by

r = r 1 e i δ 1 r 1 e i δ {\displaystyle r=-{\frac {r_{1}-e^{-i\delta }}{1-r_{1}e^{-i\delta }}}}

where r1 is the complex amplitude reflectivity of the first surface,

δ = 4 π λ n t cos θ t {\displaystyle \delta ={\frac {4\pi }{\lambda }}nt\cos \theta _{t}}
n is the index of refraction of the plate
t is the thickness of the plate
θt is the angle of refraction the light makes within the plate, and
λ is the wavelength of the light in vacuum.