| 41. | No fewer than seven interferometers have been located here.
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| 42. | Interferometers are at the core of gravitational wave detectors.
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| 43. | Both mirrors in a Michelson interferometer can be replaced with Gires Tournois etalons.
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| 44. | Schematic representation of the frequency shift when a ring laser interferometer is rotating.
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| 45. | Gires Tournois etalon has applications for laser pulse compression and nonlinear Michelson interferometer.
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| 46. | An example of an optical intensity interferometer is the Narrabri Stellar Intensity Interferometer.
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| 47. | An example of an optical intensity interferometer is the Narrabri Stellar Intensity Interferometer.
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| 48. | The use of interferometers has become a standard method of testing optical surfaces.
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| 49. | Virgo is a 3 kilometer interferometer built through a French-Italian collaboration.
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| 50. | To start with, Virgo is a Michelson interferometer whose mirrors are suspended.
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