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02 Fresnel Double Prism

Aim

To show the interference of two coherent, virtual, sources (wavefront splitting).

Subjects

Diagram

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Figure 1:.

Equipment

Presentation

Preparation

The laserbeam is switched on and expanded using a telescope consisting of the microscope objective and the converging lens of 150 mm150 \mathrm{~mm}. The expanded beam is then focussed by the lens of 50 mm50 \mathrm{~mm}.

Presentation

On the viewing screen, a couple of meters away we see a large circular light spot. (Blowing smoke into the lens set-up enlightens the light path).

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Figure 2:.

When descending the biprism (apex line vertical) into the diverging beam, close to the focal point (see Figure 2), we see that the original circular light spot is refracted into two half circle segments and that in the centre these two halves overlap (see Figure 3), narrowing the original lightspot.

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Figure 3:.

The centre shows an increase in light intensity. When the biprism is moved closer to the focal point of the 50 mm50 \mathrm{~mm} lens, we will easily see that the centre contains fringes, lines of positive and negative interference. When the biprism is close to this focal point the fringe spacing is large; when the biprism is moving away from the focal point, the fringe spacing is smaller but can still be observed when the viewing screen is tilted.

Explanation

See Figure 4. The left portion of the wavefront is refracted to the right, the right portion to the left. In the region of superposition interference occurs.

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Figure 4:.

The virtual sources S1S_{1} and S2S_{2} can be considered as separate virtual coherent sources placed a distance aa apart. The separation of the fringes ( Δy\Delta y ) is given by: Δysaλ\Delta y \approx \frac{s}{a} \lambda ( ss being the distance between the plane of the two sources and the screen).

Remarks

When the biprism approaches the focal point too close, the interference image becomes distorted. This happens largely due too the fact that we use spherical lenses in stead of cylindrical.

Sources