Michelson's interferometer played an important role in improving our understanding of light, and it has many practical uses today. For example, it may be used to measure distances precisely. Suppose themirror labeled 1 in the figure below is movable.LightsourceDetectorLA·L·SG2BIf the laser light has a wavelength of 640.0 nm, how many fringes will pass across the detector if mirror 1 is moved just 1.160 mm?fringesIf you can easily detect the passage of just one fringe, how accurately can you measure the displacement of the mirror?nm

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Answered: Michelson's interferometer played an…

University Physics Volume 3

17th Edition

ISBN:9781938168185

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Publisher:William Moebs, Jeff Sanny

Chapter4: Diffraction

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Problem 102AP: Radio telescopes are telescopes used for the detection of radio emission from space. Because radio...

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The thickness of an aluminum foil is measured using a Michelson interferometer that has its movable mirror mounted on a micrometer. There is a difference of 27 fringes in the observed interference pattern when the micrometer clamps down on the foil compared to when the micrometer is empty. Calculate the thickness of the foil?
How far apart must two objects be on the moon to be distinguishable by eye if only the diffraction effects of the eye’s pupil limit the resolution? Assume 550 nm for the wavelength of light, the pupil diameter 5.0 mm, and 400,000 km for the distance to the moon.
A telescope can be used to enlarge the diameter of a laser beam and limit diffraction spreading. The laser beam is sent through the telescope in opposite the normal direction and can then be projected onto a satellite or the moon. (a) If this is done with the Mount Wilson telescope, producing a 2.54-m-diameter beam of 633-nm light, what is the minimum angular spread of the beam? (b) Neglecting atmospheric effects, what is the size of the spot this beam would make on the moon, assuming a lunar distance of 3.84108 m?
Michelson's interferometer played an important role in improving our understanding of light, and it has many practical uses today. For example, it may be used to measure distances precisely. Suppose the mirror labeled 1 in the figure below is movable. Light source Detector V E L S G 4 B If the laser light has a wavelength of 646.0 nm, how many fringes will pass across the detector if mirror 1 is moved just 1.520 mm? fringes nm If you can easily detect the passage of just one fringe, how accurately can you measure the displacement of the mirror?
if we have. L(the distance between two mirrors ) = 15 cm A = 1.06 µm d ( the cross section radius of the absorbing media ) = lo mm n ( reflection index ) = 1.8 y = 1.5*10-3 cm Pout ( laser output power (= 150 watt R1 ( Reflectance of first mirror ) = 100% R1 (Reflectance of second mirror ) = 97% Ar ( the spectrum linewidth for atomic transition ) = 20 GHz Calcu la te : a - How many node in laser output
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What angular resolution would you expect from a pinhole with a 0.55 mm diameter?(Assume light with a wavelength of 540 nm .) Express your answer using two significant figures. να ΑΣφ ? 0min rad
Michelson's interferometer played an important role in improving our understanding of light, and it has many practical uses today. For example, it may be used to measure distances precisely. Suppose the mirror labeled 1 in the figure below is movable. If the laser light has a wavelength of 654.0 nm, how many fringes will pass across the detector if mirror 1 is moved just 1.960 (mm)? If you can easily detect the passage of just one fringe, how accurately can you measure the displacement of the mirror(nm)?
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In experiments with his interferometer, Michelson found that the red cadmium line at λ=643.8nm produced fringes until one of the arms of the interferometer was moved 25cm from initially being at the coincidence or equal path length position. a. How many fringes moved through the field of view? b. What is the approximate coherence time of the light?
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