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Michelson and Morley's interferometric setup, mounted on a stone slab that floats in an annular trough of mercury
Michelson and Morley's interferometric setup, mounted on a stone slab that floats in an annular trough of mercury
Fringe pattern produced with a Michelson interferometer using white light. As configured here, the central fringe is white rather than black.
Fringe pattern produced with a Michelson interferometer using white light. As configured here, the central fringe is white rather than black.
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