38.2 Diffraction Pattern from Narrow Slits, cont - PowerPoint PPT Presentation

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38.2 Diffraction Pattern from Narrow Slits, cont

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Left: Earth-based telescope is blurred ... and Telescope Resolution ... The Keck telescope at Mauna Kea, Hawaii, has an affective diameter of 10 m. Find ... – PowerPoint PPT presentation

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Title: 38.2 Diffraction Pattern from Narrow Slits, cont


1
38.2 Diffraction Pattern from Narrow Slits, cont
2
Intensity of Two-Slit Diffraction Patterns
  • When more than one slit is present, consideration
    must be made of
  • The diffraction patterns due to individual slits
  • The interference due to the wave coming from
    different slits
  • The single-slit diffraction pattern will act as
    an envelope for a two-slit interference pattern

3
Intensity of Two-Slit Diffraction Patterns,
Equation
  • To determine the maximum intensity
  • (38.6)
  • The factor in the square brackets represents the
    single-slit diffraction pattern
  • This acts as the envelope
  • The two-slit interference term is the cos2 term

4
Intensity of Two-Slit Diffraction Patterns, Graph
of Pattern
  • The broken blue line is the diffraction pattern
  • The red-brown curve shows the cos2 term
  • This term, by itself, would result in peaks with
    all the same heights
  • The uneven heights result from the diffraction
    term (square brackets in the equation)

5
Two-Slit Diffraction Patterns, Maxima and Minima
  • To find which interference maximum coincides with
    the first diffraction minimum
  • (38.7)
  • The conditions for the first interference
    maximum
  • d sin ? m?
  • The conditions for the first diffraction minimum
  • a sin ? ?

6
Example 38.3 Two-Slit Diffraction (Quiz 38.3)
  • Using the previous figure, make a sketch of the
    combined diffraction and interference pattern for
    650-nm light waves striking two 3.0-?m slits
    located 9.0-?m apart.
  • First case d 18.0-?m, a 3.0-?m, so m 6
  • In our case m 9/3 3.
  • The 3rd interference maximum coincides with the
    1st diffraction minimum

7
Active Figure 38.11
(SLIDESHOW MODE ONLY)
8
38.3 Resolution
  • The ability of optical systems to distinguish
    between closely spaced objects is limited because
    of the wave nature of light
  • If two sources are far enough apart to keep their
    central maxima from overlapping, their images can
    be distinguished
  • The images are said to be resolved
  • If the two sources are close together, the two
    central maxima overlap and the images are not
    resolved

9
Resolved Images, Example
  • The images are resolved
  • The images are far enough apart to keep their
    central maxima from overlapping
  • The angle subtended by the sources at the slit is
    large enough for the diffraction patterns to be
    distinguishable

10
Images Not Resolved, Example
  • The images are not resolved
  • The sources are so close together that their
    central maxima do overlap
  • The angle subtended by the sources is so small
    that their diffraction patterns overlap

11
Rayleighs Criterion
  • When the central maximum of one image falls on
    the first minimum of another image, the images
    are said to be just resolved
  • This limiting condition of resolution is called
    Rayleighs criterion

12
Rayleighs Criterion, Equation
  • The angle of separation, ?min, is the angle
    subtended by the sources for which the images are
    just resolved
  • Since ? small and sin ? ?
  • Therefore, the limiting angle (radians) of
    resolution for a slit of width a is
  • (38.8)
  • To be resolved, the angle subtended by the two
    sources must be greater than ?min

13
Circular Apertures
  • Many optical systems use circular apertures
    rather than slits
  • The diffraction pattern of a circular aperture
    consists of a central bright disk surrounded by
    progressively fainter bright and dark rings
  • The limiting angle of resolution of the circular
    aperture is
  • (38.9)
  • D is the diameter of the aperture

14
Circular Apertures, Well Resolved
  • The sources are far apart
  • The images are well resolved
  • The solid curves are the individual diffraction
    patterns
  • The dashed lines are the resultant pattern

15
Circular Apertures, Just Resolved
  • The sources are separated by an angle that
    satisfies Rayleighs criterion
  • The images are just resolved
  • The solid curves are the individual diffraction
    patterns
  • The dashed lines are the resultant pattern

16
Circular Apertures, Not Resolved
  • The sources are close together
  • The images are unresolved
  • The solid curves are the individual diffraction
    patterns
  • The dashed lines are the resultant pattern

17
Resolution, Example
  • Pluto and its moon, Charon
  • Left Earth-based telescope is blurred
  • Right Hubble Space Telescope clearly resolves
    the two objects

18
Example 38.4 Eye and Telescope Resolution
  • Estimate ?min for the human eye. Using a light
    of 500 nm and the daytime average diameter for a
    human pupil of 2.0 mm
  • The Keck telescope at Mauna Kea, Hawaii, has an
    affective diameter of 10 m. Find the resolution
    ?min for 600-nm light

19
Material for the Final Exam
  • Examples to Read!!!
  • Example 38.3 (Page 1216)
  • Homework to be solved in Class!!!
  • Problems 12, 21
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