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

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55<br />

gain, low noise, head-on photomultiplier tube. The photocathode is made <strong>of</strong> GaAs.<br />

which has a quantum efficiency <strong>of</strong> "V 14% over the range <strong>of</strong> our SHG spectroscopic<br />

measurements l.<br />

3.2 Data Acquisition<br />

The signals from the sample <strong>and</strong> reference photomultiplier tubes were sent directly<br />

to a pair <strong>of</strong> Stanford Research Systems SR530 lock-in amplifiers. The data from the<br />

lock-in amplifiers were transfered through a GPIB cable to a National Instruments<br />

AT-GPIB/TNT GPIB board in a 100 MHz Dell computer with a Pentium processor.<br />

I wrote a Quick Basic 4.5 program to graphically display, analyze, <strong>and</strong> store the<br />

data. All experiments in this thesis, with the exception <strong>of</strong> the photoluminescence<br />

experiment. acquire data in the same manner as the nonlinear spectroscopy data<br />

acquisition scheme.<br />

Prior to measuring the signals from the sample <strong>and</strong> quartz, a background measurement<br />

from both the sample <strong>and</strong> reference lines was made with the laser blocked.<br />

The appropriate background measurements were subtracted from the sample <strong>and</strong> reference<br />

signals, <strong>and</strong> a normalized signal was reported as the ratio <strong>of</strong> the sample to<br />

reference signals. In a typical nonlinear spectroscopic measurement, the lock-in amplifiers<br />

were set to a 300 ms time constant <strong>and</strong> data was acquired every second for<br />

I The R943-02 has a quantum efficiency <strong>of</strong> '" 15% at 350 nm which monotonically decreases to<br />

'" 13% at 500 nm.<br />

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

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