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01 Brewster’s Angle (1)

Aim

To show the most common source of polarized light: polarization by reflection, as observed for the first time by Etienne Malus (1808).

Subjects

Diagram

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Figure 1:.

Equipment

Presentation

Etienne Malus was standing at the window of his house in the Rue d’Enfer (Paris) examining a calcite crystal. The sun was setting, and its image reflected towards him from the windows of the Luxembourg Palace not far away. He held up the crystal and looked through it at the sun’s reflection. To his astonishment, he saw one of the double images of the sun disappear as he rotated the calcite!

This historical situation is presented in our demonstration (see Diagram). The 12Vlamp is in our situation operating at 6 V6 \mathrm{~V} in series with a 2Ω/20 W2 \Omega / 20 \mathrm{~W} resistor. This is the red glowing setting sun. The acrylic sheet is a window of the palace and the camera is the eye of Etienne Malus. The beamer projects to the audience the image that Etienne saw: “window” and reflected image of the “sun” (see Figure 2A). Take care that the camera is focussed on the light spot and not on the “window” itself.

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Figure 2:.

The lay-out of the demonstration is such that the angle of incidence is about 6060^{\circ}. The large 30609030-60-90^{\circ} triangle shows this to the students. Now the calcite crystal is placed in front of the camera-lens (see Figure 2B). Everything in the projected image is doubled. While rotating the crystal also the double images rotate, but at two positions of rotation the doubling of the reflected “sun” disappears and only one “sun” is seen!
Observe also that the double image of the window never disappears.

Explanation

In the time of Malus the birefringent action of calcite was known (see the demonstration ‘Calcite crystal’ in this database). That Malus was experimenting with such a crystal was because the French Institute had offered a prize for a mathematical theory of the double refraction. In 1821 the work of, principally Thomas Young and August Fresnel finally led to such a mathematical theory: the representation of light as some sort of transverse vibration. The so-called Fresnel equations express the effect of an incoming (plane) wave falling on an interface between two different media. These equations relate the reflected and transmitted field amplitudes to the incident amplitude:

coefficient equals: tpar =2nicosθinicosθt+ntcosθit_{\text {par }}=\frac{2 n_{i} \cos \theta_{i}}{n_{i} \cos \theta_{t}+n_{t} \cos \theta_{i}}

and tperp =2nicosθinicosθi+ntcosθtt_{\text {perp }}=\frac{2 n_{i} \cos \theta_{i}}{n_{i} \cos \theta_{i}+n_{t} \cos \theta_{t}}

Figure 3 shows these formulas in a graph (as function of the angle of incidence).

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Figure 3:.

There appears zero amplitude for rparr_{p a r} at a certain angle. This angle can be found when using Snell’s law in rpar:rpar =sinθicosθisinθtcosθtsinθicosθi+sinθtcosθtr_{p a r}: r_{\text {par }}=\frac{\sin \theta_{i} \cos \theta_{i}-\sin \theta_{t} \cos \theta_{t}}{\sin \theta_{i} \cos \theta_{i}+\sin \theta_{t} \cos \theta_{t}}. Rewriting (see textbooks) rpar =tan(θiθt)tan(θ+θiθt)r_{\text {par }}=\frac{\tan \left(\theta_{i}-\theta_{t}\right)}{\tan \left(\theta+\theta_{i} \theta_{t}\right)}

This can be zero when the denominator is infinite, so when θi+θt=90\theta_{i}+\theta_{t}=90^{\circ}. In this situation, using Snell’s law nisinθi=ntsinθtn_{i} \sin \theta_{i}=n_{t} \sin \theta_{t} yields nisinθi=ntcosθin_{i} \sin \theta_{i}=n_{t} \cos \theta_{i}, so tanθi=ntni\tan \theta_{i}=\frac{n_{t}}{n_{i}}, or θi=arctanntni\theta_{i}=\arctan \frac{n_{t}}{n_{i}}

This is Brewster’s law, formulated correctly in 1815. (Brewster was honoured half the prize of the French Institute in 1816.)

Acrylic sheet has n=1.5\mathrm{n}=1.5, so here Brewster’s angle is: θt=56\theta_{t}=56^{\circ}. This is in correspondence with our setting up of the demonstration (angle of incidence is set at about 6060^{\circ} ).

Remarks

Sources