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

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44<br />

parameter<br />

value<br />

Bl 2.35728<br />

B2 -0.01170000 J.lm- 2<br />

B3 0.01054000 J.Lm 2<br />

C 1<br />

1.34143 x 10- 4 J.Lm4<br />

C 2 -4.45368 x 10- 7 J.Lm 6<br />

C 3 5.92362x 10- 8 J.Lm 8<br />

Table 2.3: Laurent series parameters for the ordinary index <strong>of</strong> quartz [.ri].<br />

2.5 Novel Technique <strong>and</strong> Apparatus to Measure Ultrafast Pulses<br />

The analysis in the previous section suggests a technique to measure the spectral<br />

b<strong>and</strong>width <strong>of</strong> ultrafast laser pulses.<br />

Typically pulse lengths are measured by an<br />

autocorrelation technique (see section 3.4.) The autocorrelator method measures the<br />

pulse duration by a nonlinear interferometric technique [48]. The disadvantage <strong>of</strong> this<br />

technique is that it requires the interfering light pulses to be overlapped in both time<br />

<strong>and</strong> space, which is somewhat difficult to achieve in practice. If instead one measured<br />

the SHG response <strong>of</strong> a ",300 J.lm quartz wedge excited by a Ti:AI 2 0 3 ultrafast laser<br />

pulse, the damped Maker fringes could be observed. A "damping factor" may be<br />

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

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