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Figure 1. The light path through a Michelson interferometer.The two light rays with a common source combine at the half-silvered mirror to reach the detector. They may either interfere constructively (strengthening in intensity) if their light waves arrive in phase, or interfere destructively (weakening in intensity) if they arrive out of phase, depending on the exact distances between the ...
The Michelson interferometer (among other interferometer configurations) is employed in many scientific experiments and became well known for its use by Michelson and Edward Morley in the famous Michelson–Morley experiment (1887) [1] in a configuration which would have detected the Earth's motion through the supposed luminiferous aether that ...
A simple two-element optical interferometer. Light from two small telescopes (shown as lenses) is combined using beam splitters at detectors 1, 2, 3 and 4.The elements create a 1/4 wave delay in the light, allowing the phase and amplitude of the interference visibility to be measured, thus giving information about the shape of the light source.
Michelson interferometer; Mirau interferometer (also known as a Mirau objective) (microscopy) Moiré interferometer (see moiré pattern) Multi-beam interferometer ; Near-field interferometer; Newton interferometer (see Newton's rings) Nomarski interferometer; Nonlinear Michelson interferometer / Step-phase Michelson interferometer; N-slit ...
An astronomical interferometer or telescope array is a set of separate telescopes, mirror segments, or radio telescope antennas that work together as a single telescope to provide higher resolution images of astronomical objects such as stars, nebulas and galaxies by means of interferometry.
Because the scatterplate interferometer is a common-path interferometer, the reference and test paths are automatically matched so that a zero order fringe can be easily obtained even with white light. It is relatively insensitive to vibration and turbulence, and the quality of the auxiliary optics is not as critical as in a Twyman-Green setup ...
The interferometer consists of two mirrors, made of the thickest glass possible. The Fresnel reflection from the first surface of the mirror acts as a beam splitter . The incident light is split into two rays, parallel to each other and displaced by an amount depending on the thickness of the mirror.
Both arms of the interferometer were contained in a transparent solid . The light source was a Helium–neon laser. ~7 km/s Trimmer et al. [30] [31] 1973: They searched for anisotropies of the speed of light behaving as the first and third of the Legendre polynomials. They used a triangle interferometer, with one portion of the path in glass.