The Arcminute Microkelvin Imager consists of a pair of interferometric radio telescopes - the Small and Large Arrays - located at the Mullard Radio Astronomy Observatory near Cambridge. AMI was design
The 8 antennas of the Arcminute Microkelvin Imager Large Array viewed from Barton Road in 2012
AMI Large Array in June 2014
AMI Large Array silhouette in 2020
Interferometry is a technique which uses the interference of superimposed waves to extract information. Interferometry typically uses electromagnetic waves and is an important investigative technique
Figure 11. The VLA interferometer
ALMA is an astronomical interferometer located in Chajnantor Plateau
Figure 13. Optical flat interference fringes. (left) a flat surface, indicated by a pattern of straight parallel interference fringes at equal intervals; (right) curved surface.
Figure 18. Lunate cells of Nepenthes khasiana visualized by Scanning White Light Interferometry (SWLI)