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Light

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Light and other Electromagnetic Radiation Radiation A loaded term; That which makes radiation dangerous is primarily its energy; Energy is related to wavelength ... – PowerPoint PPT presentation

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Title: Light


1
Light
  • and other Electromagnetic Radiation

2
Radiation
  • A loaded term
  • That which makes radiation dangerous is primarily
    its energy
  • Energy is related to wavelength low frequency,
    long wavelength, low energy.
  • Length of exposure, proximity to the source is
    also important.

3
The Electromagnetic Spectrum
  • Wavelengths ranging from 10,000 m (and longer) to
    0.000,000,000,000,01 m (and shorter).

4
Danger!
  • Pretty safe up through visible light (unless you
    stick your head in a microwave oven!).
  • Pretty much dangerous from Ultraviolet and
    shorter.

5
Sources of EM Radiation
  1. Antennae
  2. Atomic orbitals
  3. Atomic nucleus

6
Antennae
  • Electrons (or any charged particle) emit electric
    fields.
  • Moving charges make magnetic fields,
  • so moving charges emit electromagnetic radiation.
  • Mostly longer wavelength Marine radio to
    microwaves.

7
Atomic Orbitals
  • For all atoms hydrogen illustrated.
  • When an atoms electron absorbs the right amount
    of energy, it will move to a higher energy level,
    a higher orbit about its nucleus.
  • After a billionth of a second or so it falls back
    down to the initial or ground state.

8
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9
Photons
  • As the electron drops back down to the ground
    state, it emits a photon (particle of light) with
    a wavelength directly dependent on the energy of
    the jump.
  • These jumps to ground yield wavelengths too short
    to be seen (ultraviolet).
  • However, when they land on the second level (n
    2), the result is a discreet spectra.

10
Emission Spectrum
11
Atomic Nucleus
  • Very high energy photon from an atomic nucleus
    breaking apart.
  • Takes some of that E mc2 for its energy.
  • Hard X-Rays and Gamma rays.
  • Even higher radiation comes from exploding stars
    (supernovae) cosmic rays.

12
The Particle/Wave Duality
  • Huygens 1650 light is a wave
  • Newton 1700 light is a particle
  • Young 1800 light is a wave
  • Planck1900 light is a particle
  • Its both! A particle of light (photon) has wave
    characteristics.

13
Optics
  • Geometric Optics
  • Physical Optics

14
Images
  • Real (can be projected) or virtual (in the
    mirror)
  • Erect (right-side up) or inverted
  • Magnified (bigger) or diminished (smaller)

15
Geometric Optics Mirrors
  • Plane (flat) mirrors virtual image, erect,
    magnification of 1.
  • Concave (curved inward). Like a makeup mirror.
    Inside the focal length (1/2 the radius of the
    curve) the image is virtual, erect and bigger.
    Outside its smaller, inverted, and real.
  • Convex (curved outward). Passenger side mirror.
    Images are virtual, erect, and smaller.

16
Index of Refraction
  • Light travels at 186,000miles per second in a
    vacuum, but slower in everything else.
  • In the process of slowing down as it enters
    water, glass, etc., the light beam bends inward.
  • When it exits, it speeds up and bends away.
  • The amount of bending depends on the Index of
    Refraction, the ratio of the speed of light in a
    vacuum to its speed in a medium.
  • Can be used to make lenses, prisms, etc.

17
Lenses
  • Flat (like a window)
  • Concave (diverging). Spreads light waves.
  • Corrects near-sightedness
  • Convex (converging). Focuses rays to a point.
  • Corrects far-sightedness.

18
Prisms
  • Different wavelengths (colors) of light have
    different speeds in a medium. This causes them to
    bend different.
  • White light is composed of all colors a prism
    separates them.

19
Famous Album Cover
20
Total Internal Reflection
  • When light tries to escape from a medium, if the
    angle is too great then it is completely
    reflected back down.
  • (the explanation requires trig!!)
  • Circle of seeing for fish and divers looking
    up.
  • The physics behind fiber optics.

21
Physical Optics
  • Diffraction
  • Polarization

22
Diffraction
  • The bending of light around corners.
  • When any wave encounters an edge, it bends around
    it.
  • Light will spread out through a thin slit in
    otherwise opaque material.

23
LASER
  • Light Amplification by Stimulated Emission of
    Radiation.
  • Useful for many things especially for
    diffraction demonstrations.
  • Exactly one color of light that doesnt spread
    out (much).

24
Interference
  • When a slit causes light to bend, the distance
    from one edge to a far-off wall could be ½ a
    wavelength different from the distance from the
    other edge.
  • Therefore, one wave may be up while the other
    wave may be down.
  • The interfere destructively (cancel out)
  • If both waves are NSync (sorry) then they
    interfere constructively (add up)

25
Fringe Patterns
  • The pattern of light and dark spots on the wall
    made by a LASER beamed through a slit.
  • The reason? Diffraction and Interference!
  • Gratings can also be used to separate colors,
    since the amount of bending depends on the
    lights wavelength.

26
Polarization
  • Light from most sources is disorganized.
  • The plane of each wave is randomly oriented to
    each other. Think of many airplanes flying with
    different tilts to their wings unpolarized.
  • A polarizing filter will allow only the correctly
    oriented waves through, lining them all up
    polarized.
  • Two filters at 90o will block light altogether!
  • Good in sunglasses for blocking glare, which is
    polarized.
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