Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Interferometry
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Basic principles== [[File:Michelson interferometer fringe formation.svg|thumb|300px|Figure 2. Formation of fringes in a Michelson interferometer]] [[File:Colored and monochrome fringes.png|thumb|225px|Figure 3. Colored and monochromatic fringes in a Michelson interferometer: (a) White light fringes where the two beams differ in the number of phase inversions; (b) White light fringes where the two beams have experienced the same number of phase inversions; (c) Fringe pattern using monochromatic light ([[Fraunhofer lines|sodium D lines]])]] {{further|Interference (wave propagation)}} Interferometry makes use of the principle of superposition to combine waves in a way that will cause the result of their combination to have some meaningful property that is diagnostic of the original state of the waves. This works because when two waves with the same [[frequency]] combine, the resulting intensity pattern is determined by the [[phase (waves)|phase]] difference between the two wavesโwaves that are in phase will undergo constructive interference while waves that are out of phase will undergo destructive interference. Waves which are not completely in phase nor completely out of phase will have an intermediate intensity pattern, which can be used to determine their relative phase difference. Most interferometers use [[light]] or some other form of [[electromagnetic wave]].<ref name=HariharanBasics2007/>{{rp|3โ12}} Typically (see Fig. 1, the well-known Michelson configuration) a single incoming beam of [[coherence (physics)|coherent]] light will be split into two identical beams by a [[beam splitter]] (a partially reflecting mirror). Each of these beams travels a different route, called a path, and they are recombined before arriving at a detector. The path difference, the difference in the distance traveled by each beam, creates a phase difference between them. It is this introduced phase difference that creates the interference pattern between the initially identical waves.<ref name=HariharanBasics2007/>{{rp|14โ17}} If a single beam has been split along two paths, then the phase difference is diagnostic of anything that changes the phase along the paths. This could be a physical change in the [[Optical path length|path length]] itself or a change in the [[refractive index]] along the path.<ref name=HariharanBasics2007/>{{rp|93โ103}} As seen in Fig. 2a and 2b, the observer has a direct view of mirror ''M''<sub>1</sub> seen through the beam splitter, and sees a reflected image ''{{prime|M}}''<sub>2</sub> of mirror ''M''<sub>2</sub>. The fringes can be interpreted as the result of interference between light coming from the two virtual images ''{{prime|S}}''<sub>1</sub> and ''{{prime|S}}''<sub>2</sub> of the original source ''S''. The characteristics of the interference pattern depend on the nature of the light source and the precise orientation of the mirrors and beam splitter. In Fig. 2a, the optical elements are oriented so that ''{{prime|S}}''<sub>1</sub> and ''{{prime|S}}''<sub>2</sub> are in line with the observer, and the resulting interference pattern consists of circles centered on the normal to ''M''<sub>1</sub> and ''M'<sub>2</sub>''. If, as in Fig. 2b, ''M''<sub>1</sub> and ''{{prime|M}}''<sub>2</sub> are tilted with respect to each other, the interference fringes will generally take the shape of conic sections (hyperbolas), but if ''{{prime|M}}''<sub>1</sub> and ''{{prime|M}}''<sub>2</sub> overlap, the fringes near the axis will be straight, parallel, and equally spaced. If S is an extended source rather than a point source as illustrated, the fringes of Fig. 2a must be observed with a telescope set at infinity, while the fringes of Fig. 2b will be localized on the mirrors.<ref name=HariharanBasics2007/>{{rp|17}} Use of white light will result in a pattern of colored fringes (see Fig. 3).<ref name=HariharanBasics2007/>{{rp|26}} The central fringe representing equal path length may be light or dark depending on the number of phase inversions experienced by the two beams as they traverse the optical system.<ref name=HariharanBasics2007/>{{rp|26,171โ172}} (See [[Michelson interferometer#Configuration|Michelson interferometer]] for a discussion of this.)
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Interferometry
(section)
Add topic