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

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22<br />

the transmitted wave, E:t'°,<br />

The measured signal, I:t'° is<br />

(2.21)<br />

where<br />

(2.22)<br />

vVe observed Maker fringes by measuring the SHG intensity from a quartz wedge<br />

excited by aNd: YAG pumped dye laser. By translating the quartz wedge through<br />

the dye laser light, the phase difference between the bound <strong>and</strong> free waves changes<br />

as the quartz thickness changes. Fig. 2.3 demonstrates the simplified experimental<br />

geometry used to observe Maker fringes [411. Fig. 2.4 displays the Maker fringe data<br />

<strong>and</strong> a fit to the data using equation (2.21). The salient feature <strong>of</strong> this fitting function<br />

is that the intensity oscillates as a function <strong>of</strong> the phase velocity mismatch, (k bl - k /1),<br />

times the crystal thickness, d.<br />

2.4.2 Excitation with a Ultrafast Light Source<br />

In linear optics, propagation <strong>of</strong> ultrafast laser pulses in dispersive media depends in<br />

part on group velocity dispersion (GVD). In this phenomena, an ultrafast laser pulse<br />

is broadened as it traverses a dispersive media. The pulse broadens more rapidly when<br />

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

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