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presents
a                 production




    Resolution
          1
Circular aperture


Light diffracted by a circular aperture forms a pattern
  of concentric rings with a bright ‘Airy disc’ in the
centre. Examples of circular apertures are the pupil of
    the eye; a camera lens; a radio telescope dish.
                                                  Image: livjm.ac.uk
Diffraction patterms

                                               Diffraction by circular
    Diffraction by slit of width b            aperture of diameter b

                                                  Average diameter
                     In both cases, angle is      of circle = b/1.22
                proportional to wavelength and
                 inversely proportional to slit
                             width.
Image: photoresearchers                                                Image: oberlin
Resolution
      Light passing through an aperture is diffracted. If
       the images of two objects viewed through the
         aperture are so close that their diffraction
      patterns overlap, they will be difficult to resolve.

                                   Resolution is the ability
                                     to distinguish two
                                      separate images.

                                  These illuminated objects
                                  can be resolved because
                                their Airy discs are separate.
Image: NHMFL
Rayleigh criterion                               Image: NHMFL
The limit of resolvability is
  when the middle of the
 central maximum of one
 image coincides with the
   first minimum of the
  other. At this limit, the
  angle subtended by the
  two points is given by:
                                 where b is the diameter of
                                the aperture through which
  The Rayleigh criterion          the objects are viewed.
Better resolution
     Better resolution means that
    the angle is as small as possible.
   This is achieved by using a large
   aperture or a short wavelength.
  Thus, big lenses resolve better than
  small ones and the eye can resolve
  violet light better than red because
there is less diffraction at the aperture.
Resolution problems
A light telescope has a circular mirror of radius 127 cm.
What is the smallest angle it can resolve for light of
wavelength 550 nm? [264 nrad]
Two stars are 20 ly distant and can just be resolved using
a telescope with aperture of 55 cm. How far apart are
the stars? Assume light of wavelength 450 nm.
[11.5 light-minutes]
Two spotlights are 12 m apart. How far away can a
human eye (pupil diameter 0.40 cm) distinguish the
spotlights if the wavelength of the light is 620 nm?
[63 km]
Resolution examples
CDs and DVDs use reflection of laser light from ‘pits’ on
the surface. To store more information, the pits must be
smaller, but there is a limit to resolvability. One solution
is to use shorter wavelength light.
If the object is too small, a light microscope cannot
resolve it due to diffraction at the lens; below uv
(400nm) the light as not visible. An electron microscope
uses electrons with wavelengths of 0.2 nm.
Radio telescopes detect radio waves from space. Since
these have a long wavelength, and are hard to resolve,
the radius of the dishes of the telescopes is huge.
Where these two gold
crystals meet they are
joined by a complex
arrangement of atoms,
forming a nano-bridge.
The atoms are 2.3
angstroms apart. This       Image from Hubble
resolution is possible       Space Telescope of
due to electron          binary star system just
microscopy.               resolved. It is 8 000 ly
                               away and a third
                              unresolved star is
                                      suspected.
a                                          production




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IB Physics Resolution flippingphysics by Nothingnerdy

  • 1. presents a production Resolution 1
  • 2. Circular aperture Light diffracted by a circular aperture forms a pattern of concentric rings with a bright ‘Airy disc’ in the centre. Examples of circular apertures are the pupil of the eye; a camera lens; a radio telescope dish. Image: livjm.ac.uk
  • 3. Diffraction patterms Diffraction by circular Diffraction by slit of width b aperture of diameter b Average diameter In both cases, angle is of circle = b/1.22 proportional to wavelength and inversely proportional to slit width. Image: photoresearchers Image: oberlin
  • 4. Resolution Light passing through an aperture is diffracted. If the images of two objects viewed through the aperture are so close that their diffraction patterns overlap, they will be difficult to resolve. Resolution is the ability to distinguish two separate images. These illuminated objects can be resolved because their Airy discs are separate. Image: NHMFL
  • 5. Rayleigh criterion Image: NHMFL The limit of resolvability is when the middle of the central maximum of one image coincides with the first minimum of the other. At this limit, the angle subtended by the two points is given by: where b is the diameter of the aperture through which The Rayleigh criterion the objects are viewed.
  • 6. Better resolution Better resolution means that the angle is as small as possible. This is achieved by using a large aperture or a short wavelength. Thus, big lenses resolve better than small ones and the eye can resolve violet light better than red because there is less diffraction at the aperture.
  • 7. Resolution problems A light telescope has a circular mirror of radius 127 cm. What is the smallest angle it can resolve for light of wavelength 550 nm? [264 nrad] Two stars are 20 ly distant and can just be resolved using a telescope with aperture of 55 cm. How far apart are the stars? Assume light of wavelength 450 nm. [11.5 light-minutes] Two spotlights are 12 m apart. How far away can a human eye (pupil diameter 0.40 cm) distinguish the spotlights if the wavelength of the light is 620 nm? [63 km]
  • 8. Resolution examples CDs and DVDs use reflection of laser light from ‘pits’ on the surface. To store more information, the pits must be smaller, but there is a limit to resolvability. One solution is to use shorter wavelength light. If the object is too small, a light microscope cannot resolve it due to diffraction at the lens; below uv (400nm) the light as not visible. An electron microscope uses electrons with wavelengths of 0.2 nm. Radio telescopes detect radio waves from space. Since these have a long wavelength, and are hard to resolve, the radius of the dishes of the telescopes is huge.
  • 9. Where these two gold crystals meet they are joined by a complex arrangement of atoms, forming a nano-bridge. The atoms are 2.3 angstroms apart. This Image from Hubble resolution is possible Space Telescope of due to electron binary star system just microscopy. resolved. It is 8 000 ly away and a third unresolved star is suspected.
  • 10. a production MUCH MORE AT http://nothingnerdy.wikispaces.com http://nothingnerdy.wikispaces.com/11.4+Resolution 10

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