A 0.54-mm-diameter hole is illuminated by light ofwavelength 530 nm.Part AWhat is the width (in mm) of the central maximum on a screen 1.8 m behind the slit?Express your answer in millimeters.ΜΕ ΑΣΦ?Q4NFZF3@2#3$4455%SubmitRequest AnswerProvide FeedbackFS^6F687WERTYUSD-l(89-mm44F10ΟDFGHJKLP<259)F12={[]12?XCVBNMHH\commandoptioncommandNext>delete

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A 0.54-mm-diameter hole is illuminated by light of wavelength 530 nm. Part A What is the width (in mm) of the central maximum on a screen 1.8 m behind the slit? Express your answer in millimeters. ΜΕ ΑΣΦ ? 2 14/ 2 #3 Submit Request Answer Provide Feedback a 76 20 23 2 54 25 6 7 &フ mm 10 D 99 1 910 912 8 9 Next> delete

A 0.54-mm-diameter hole is illuminated by light of wavelength 530 nm. Part A What is the width (in mm) of the central maximum on a screen 1.8 m behind the slit? Express your answer in millimeters. ΜΕ ΑΣΦ ? 2 14/ 2 #3 Submit Request Answer Provide Feedback a 76 20 23 2 54 25 6 7 &フ mm 10 D 99 1 910 912 8 9 Next> delete

University Physics Volume 3

17th Edition

ISBN:9781938168185

Author:William Moebs, Jeff Sanny

Publisher:William Moebs, Jeff Sanny

Chapter3: Interference

Section: Chapter Questions

Problem 63AP: A hydrogen gas discharge lamp emits visible light at four wavelengths, =410 , 434, 486, and 656 nm....

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Similar questions

A hydrogen gas discharge lamp emits visible light at four wavelengths, =410 , 434, 486, and 656 nm. (a) If light from this lamp falls on a N slits separated by 0.025 mm, how far from the central maximum are the third maxima when viewed on a screen 2.0 m from the slits? (b) By what distance are the second and third maxima separated for l=486 nm?
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?
Fifty-one narrow slits are equally spaced and separated by 0.10 mm. The slits are illuminated by blue light of wavelength 400 nm. What is angular position of the twenty-fifth secondary maximum? What is its peak intensity in comparison with that of the primary maximum?
A 5.08-cm-long rectangular glass chamber is inserted into one arm of a Michelson interferometer using a 633-nm light source. This chamber is initially filled with air (n=1.000293) at standard atmospheric pressure but the air is gradually pumped out using a vacuum pump until a near perfect vacuum is achieved. How many fringes are observed moving by during the transition?
X-rays of wavelength 0.103 nm reflects off a crystal and a second-order maximum is recorded at a Bragg angle of 25.5°. What is the spacing between the scattering planes in this crystal?
If 500-nm and 650-nm light illuminates two slits that are separated by 0.50 mm, how far apart are the second-order maxima for these two wavelengths on a screen 2.0 m away?
A monochromatic light of wavelength 589 nm incident on a double slit with slit width 2.5 m and unknown separation results in a diffraction pattern containing nine interference peaks inside the central maximum. Find the separation of the slits.
What is the separation between two slits for which 610-nm orange light has its first maximum at an angle of 30.0°?
Radio telescopes are telescopes used for the detection of radio emission from space. Because radio waves have much longer wavelengths than visible light, the diameter of a radio telescope must be very large to provide good resolution. For example, the radio telescope in Penticton, BC in Canada, has a diameter of 26 m and can be operated at frequencies as high as 6.6 GHz. (a) What is the wavelength corresponding to this frequency? (b) What is the angular separation of two radio sources that can be resolved by this telescope? (c) Compare the telescope’s resolution with the angular size of the moon.
Calculate the wavelength of light that produces its first minimum at an angle of 36.9° when falling on a single slit of width 1.00 m.
Suppose you have a lens system that is to be used primarily for 700-nm red light. What is the second thinnest coating of fluorite (magnesium fluoride) that would be nonreflective for this wavelength?
What is the smallest separation between two slits that will produce a second-order maximum for 720-nm red light?