16. Finally, we are going to use the measured positions of dark fringes to calculate an unknown wavelength of light that is diffracting through a single slit. For these calculations, assume a slit width of a = 0.02 mm, and a distance of exactly L = 1.00 m between the screen and the slit. P 1 2 3 4 YR (mm) 20.03 39.98 60.00 80.10 0, (radians) λ (nm)
16. Finally, we are going to use the measured positions of dark fringes to calculate an unknown wavelength of light that is diffracting through a single slit. For these calculations, assume a slit width of a = 0.02 mm, and a distance of exactly L = 1.00 m between the screen and the slit. P 1 2 3 4 YR (mm) 20.03 39.98 60.00 80.10 0, (radians) λ (nm)
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![16. Finally, we are going to use the measured positions of dark fringes to calculate an unknown
wavelength of light that is diffracting through a single slit. For these calculations, assume a
slit width of a = 0.02 mm, and a distance of exactly L = 1.00 m between the screen and
the slit.
P
1
2
3
4
13022
YR (mm)
20.03
39.98
60.00
80.10
BREAU
0, (radians)
120303
λ (nm)](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F28ab91b5-1c00-4abd-9133-93550dcbd19f%2F5ba48e6a-1154-4e24-bc42-a93ce6f3f8f2%2Fsehxb5_processed.jpeg&w=3840&q=75)
Transcribed Image Text:16. Finally, we are going to use the measured positions of dark fringes to calculate an unknown
wavelength of light that is diffracting through a single slit. For these calculations, assume a
slit width of a = 0.02 mm, and a distance of exactly L = 1.00 m between the screen and
the slit.
P
1
2
3
4
13022
YR (mm)
20.03
39.98
60.00
80.10
BREAU
0, (radians)
120303
λ (nm)
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