he diffraction grating is a way of separating or dispersing light of different wavelengths, producing a spectrum of light. The grating interferes light constructively in particular directions: dsinθm=mλdsin⁡θm=mλ For a particular angle, we calculate the wavelength. The grating constant (or line density) is 500 lines per mm -- every millimeter has 500 lines scratched onto it, equally spaced. The quantity d is the distance between the lines, and λ is the light wavelength. A meter stick shows the spots, and ym is position on the meter stick of the mth-order light beam. (Negative order is the same as positive order.) Calculate the light wavelength, λ in nm, given this information: The grating constant is 500 lines/mm. L = 31.5 cm y1 = 56.9 cm y-1 = 40.8 cm y0 isn't specified because of computer issues. (It's the average of y1 and y-1.)

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Chapter1: Units, Trigonometry. And Vectors
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The diffraction grating is a way of separating or dispersing light of different wavelengths, producing a spectrum of light.  The grating interferes light constructively in particular directions:

dsinθm=mλdsin⁡θm=mλ 

For a particular angle, we calculate the wavelength.

The grating constant (or line density) is 500 lines per mm -- every millimeter has 500 lines scratched onto it, equally spaced.  The quantity d is the distance between the lines, and λ is the light wavelength.

 

A meter stick shows the spots, and ym is position on the meter stick of the mth-order light beam.  (Negative order is the same as positive order.)  Calculate the light wavelength, λ in nm, given this information:

  • The grating constant is 500 lines/mm.
  • L = 31.5 cm
  • y1 = 56.9 cm
  • y-1 = 40.8 cm
  • y0 isn't specified because of computer issues.  (It's the average of y1 and y-1.)
 
y2
grating/6, L
Yo
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Y-1
Y-2
Transcribed Image Text:y2 grating/6, L Yo Laser Y-1 Y-2
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