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William Angerer - Department of Physics and Astronomy - University ...

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42<br />

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iii iii iii iii iii iii iii Iii iii iii iii i<br />

I<br />

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«<br />

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~<br />

en<br />

C<br />

Q)<br />

--c<br />

(!)<br />

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2000<br />

~<br />

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O~~~~~~~~~~~~~~~~~~~~~LW<br />

o 100 200 300 400 500<br />

Quartz Thickness (,urn)<br />

Figure 2.8: Calculated ~laker fringes with a broadb<strong>and</strong> source as a function <strong>of</strong> quartz<br />

thickness. The light generating source is a Ti:AI 2 0 3 laser. The ~laker fringes damp<br />

out as the quartz slab gets thicker.<br />

the material becomes more dispersive. or the pulse duration <strong>of</strong> the laser decreases.<br />

i.e. the b<strong>and</strong>width increases.<br />

;..iote. the index <strong>of</strong> refraction <strong>and</strong> the group velocity were derived from the Laurent<br />

expression for the ordinary index <strong>of</strong> refraction <strong>of</strong> quartz<br />

(2.67)<br />

The parameters for equation (2.67) are displayed in Table 2.3.<br />

Reproduced with permission <strong>of</strong> the copyright owner. Further reproduction prohibited without permission.

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