Physics 30 - Unit C: Chapter 13.4

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21 Terms

1
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Refraction

The change in direction of waves at the boundary between two different media.

  • this change in direction is caused by a change in

    speed

<p>The <strong><u>change in direction</u></strong> of waves at the boundary between <u>two different media</u>.</p><ul><li><p>this <em>change in direction</em> is caused by a <em>change in</em></p><p><em>speed</em></p></li></ul><p></p>
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Refractive Index Equation

The more optically dense the medium, the slower light will travel through it.

  • refractive index of a medium (n)

  • speed of light in a vacuum (c)

  • speed of light measured in the medium (v)

<p>The <strong><u>more optically dense the medium</u></strong>, the <strong><u>slower light will travel</u></strong> through it.</p><ul><li><p>refractive index of a medium <strong>(n)</strong></p></li><li><p>speed of light in a vacuum <strong>(c)</strong></p></li><li><p>speed of light measured in the medium <strong>(v)</strong></p></li></ul><p></p>
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Index of Refraction Chart

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Light Travelling From Low → High Refractive Index

When light travels from a medium with a low refractive index to a higher refractive index, it slows down and bends toward the normal.

<p>When light travels from a medium with a <em>low refractive index to a higher refractive index</em>, <strong><u>it slows down and bends toward the normal.</u></strong></p>
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Light Travelling From High → Low Refractive Index

When light travels from a medium with a higher refractive index to a medium with a lower refractive index, it speeds up and bends away from the normal.

<p>When light travels from a medium with a <em>higher refractive index to a medium with a lower refractive index</em>,<strong> <u>it speeds up and bends away from the normal.</u></strong></p>
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Universal Wave Equation

  • frequency of the source (f in Hz)

  • wavelength (λ)

Wavelength and Frequency have an inverse relationship.

  • source frequency is high = wavelength is short

  • source frequency is low = wavelength is long

<ul><li><p>frequency of the source <strong>(f in Hz)</strong></p></li><li><p>wavelength <strong>(λ)</strong></p></li></ul><p><em>Wavelength</em> and <em>Frequency</em> have an <strong><u>inverse relationship.</u></strong></p><ul><li><p>source <u>frequency is </u><strong><u>high</u> </strong>= <u>wavelength is </u><strong><u>short</u></strong></p></li><li><p>source <u>frequency is </u><strong><u>low</u></strong> = <u>wavelength is </u><strong><u>long</u></strong></p></li></ul><p></p>
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Snell’s Law of Refraction

For any ray that passes from air (θair) into a second medium (θr , refractive index n):

If the first medium is not air, then the general form applies:

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Snell’s Law, Refraction and Wavelength

Light are transverse waves, it obeys the universal wave equation.

  • if frequency is constant, a change in speed would correspond with a change in wavelength

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*IMPORTANT FACT ABOUT FREQUENCY*

As a wave moves from one medium to another, there is no change in frequency.

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Total Internal Reflection

Reflection of all the incident light back into a medium of higher refractive index due to the inability to refract light beyond the maximum angle of 90°.

<p>Reflection of all the incident light back into a medium of higher refractive index due to the inability to refract light beyond the maximum angle of 90°.</p>
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Critical Angle

The critical angle for any two media is the angle of incidence for which the angle of refraction is 90°.

  • to find critical angle, set angle of refraction to 90° → solve for angle of incidence

<p>The critical angle for any two media is the angle of incidence for which the angle of refraction is 90°.</p><ul><li><p>to find critical angle, set angle of refraction to 90° → solve for angle of incidence</p></li></ul><p></p>
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Prisms – Dispersion of White Light

White light is a mixture of a spectrum of colours: R O Y G B V

  • in order of increasing frequency = decreasing wavelength

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Dispersion

The separation of white light into its components.

  • the lower the wavelength of light → the more it refracts

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Converging (Convex) Lens

refract rays that are parallel to the principal axis through the real principal focal point.

<p>refract rays that are parallel to the principal axis through the <strong>real principal focal point</strong>.</p>
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Diverging (Concave) Lens

refracts rays that are parallel to the principal axis so they appear to diverge from the virtual principal focal point.

<p>refracts rays that are parallel to the principal axis so they appear to <strong>diverge</strong> from the <strong>virtual principal focal point</strong>.</p>
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Principal Plane

a line that is perpendicular to the principal axis, through the centre of the lens.

<p>a line that is <strong>perpendicular to the principal axis</strong>, through the <em>centre of the lens.</em></p>
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Optical Centre

the intersection point between the principal plane and the principal axis.

<p>the <strong><u>intersection point between</u></strong> the <em>principal plane</em> and the <em>principal axis</em>.</p>
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Drawing Ray Diagrams for Converging Lenses

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Drawing Ray Diagrams for Diverging Lenses

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Equation for Thin Lenses

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Sign Conventions for Use with the Thin Lens Equation

  • All distance measurements are relative to the optical center of the lens.

  • Positive Distance = real images.

  • Negative Distances = virtual images.

  • Positive Image Heights = above principal axis.

  • Negative Image Heights = below principal axis.

  • Converging Lenses = positive focal length.

  • Diverging Lenses = negative focal length.