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Figure 1. A basic Michelson interferometer, not including the optical source and detector.
Figure 1. A basic Michelson interferometer, not including the optical source and detector.
This photo shows the fringe pattern formed by the Michelson interferometer, using monochromatic light (sodium D lines).
This photo shows the fringe pattern formed by the Michelson interferometer, using monochromatic light (sodium D lines).
Figure 9. Magnetogram (magnetic image) of the Sun showing magnetically intense areas (active regions) in black and white, as imaged by the Helioseismi
Figure 9. Magnetogram (magnetic image) of the Sun showing magnetically intense areas (active regions) in black and white, as imaged by the Helioseismic and Magnetic Imager (HMI) on the Solar Dynamics Observatory
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Figure 11. The VLA interferometer
Figure 11. The VLA interferometer
ALMA is an astronomical interferometer located in Chajnantor Plateau
ALMA is an astronomical interferometer located in Chajnantor Plateau
Figure 13. Optical flat interference fringes. (left) flat surface, (right) curved surface.
Figure 13. Optical flat interference fringes. (left) flat surface, (right) curved surface.
Figure 18. Lunate cells of Nepenthes khasiana visualized by Scanning White Light Interferometry (SWLI)
Figure 18. Lunate cells of Nepenthes khasiana visualized by Scanning White Light Interferometry (SWLI)