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CLIOwin 7 PCI User's Manual - Audiomatica

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it is necessary to remove the flight time plus the device settling time; this can be easily<br />

accomplished setting the internal trigger delay, in FFT settings, to 1.5ms; the final result<br />

shown is shown in 11.11 and permits the identification of the device harmonic distortion.<br />

To proceed further one could vary the stimulus amplitude and test the distortion of the<br />

tweeter at different amplitudes; using bursts also prevents the damage of the unit as<br />

the overall power delivered to it rather low and a direct function of the duty cycle of the<br />

burst itself.<br />

The main application of RTA analysis is in assessing the quality of an audio installation<br />

(from the placement of the speakers in a listening room to the overall sound quality of<br />

a car stereo system). In these cases pink noise is often used as the stimulus. If you<br />

are not using CLIO as the source of such a stimulus be sure to use a good one; you<br />

may find several audio generators that do the job, but they are usually expensive. A<br />

good choice is to use a recorded track of one of the various test CDs available; in this<br />

case not all the CD-ROM readers may furnish adequate results, as appears from the<br />

graph in Fig.9.3<br />

0.0<br />

CLIO<br />

dBV<br />

-20.0<br />

-40.0<br />

-60.0<br />

-80.0<br />

-100.0<br />

20 100 1k Hz<br />

10k 20k<br />

Figure 9.3<br />

All three graphs represent true analog pink noise, they are played at intervals of 5dB<br />

for clarity. The upper (red) is the output of an Audio Precision System One generator;<br />

the second (blue) is the pink noise of track 4 of the Stereophile Test CD played by a<br />

Philips CD692 CD player, the third is the same track of the same test CD output by the<br />

computer which I'm writing with right now (Pioneer DVD Player plus Crystal Sound<br />

Fusion <strong>PCI</strong> Audio).<br />

When taking RTA measurements use, at least, 16k FFT size if you want to cover<br />

the entire 20-20kHz audio band; using lower sizes results in octave bands not<br />

present as no FFT bins fall inside them.<br />

100 Chapter 9 - FFT

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