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Wave propagation.

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Wave propagation. Aims: Huygen s Principle: Reflection and refraction. Problems Huygen s-Fresnel principle Fraunhofer diffraction (waves in the far field ). – PowerPoint PPT presentation

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Title: Wave propagation.


1
Lecture 9
  • Wave propagation.
  • Aims
  • Huygens Principle
  • Reflection and refraction.
  • Problems
  • Huygens-Fresnel principle
  • Fraunhofer diffraction (waves in the far
    field).
  • Youngs double slits
  • Three slits
  • N slits and diffraction gratings
  • A single broad slit
  • General formula - Fourier transform.

This lecture
2
Huygens Principle
  • Remember the concept of wavefront - a surface of
    constant phase.
  • 1690 Treatise on light, Huygens.
  • Every point of a primary wavefront behaves as
    the source of spherical, secondary wavelets, such
    that the primary wavefront at a later time is the
    envelope of these wavelets the wavelets have the
    same frequency and velocity as the incoming wave
  • Rectilinear propagation
  • Spherical propagation

3
Reflection and refraction
  • qr qi
  • Result follows from the 2 right-angled triangles
    with same hypotenuse, both having one side of
    length vt. Thus qr qi.
  • Snells Law

4
Huygens-Fresnel principle
  • Shortcomings It is easy to criticise Huygens
  • No theoretical basis
  • Why neglect parts of the wavelet other than those
    forming the envelope
  • Why dont wavelets propogate backwards
  • It is no help in predicting amplitudes etc...
  • None detract from its historical significnce and
    the fact that it works.
  • Fresnel (1818) (See handout).
  • He built in Youngs concept of interference.
    Every unobstructed point of a wavefront serves
    as a source of spherical secondary wavelets The
    amplitude of the optical field at any point
    beyond is the superposition of all these wavelets
    (considering their amplitudes and relative
    phases)
  • Note backward travelling wavelets tend to
    interfere destructively
  • Kirchoff (1824-1887)
  • Provided theoretical foundation by connecting the
    wave equation to a surface integral of spherical
    wavelets.
  • See Optics course, next term.
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