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User Manual - TRS-RenTelco

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Option SD/HD Detailed Measurement Information<br />

this example). If the extra spectral content is removed by filtering, the resulting<br />

sinusoid will have the amplitude shown in the results.<br />

Generally, if the signal has undergone processing without a required anti-alias<br />

filter (as in re-sampling for format conversion, or signal reconstruction), each<br />

burst may contain one or several frequency aliases. In such cases, burst<br />

frequencies that increase with each burst of the input signal may contain burst<br />

frequencies in nearly any order in the output of the device under test.<br />

For example, in the 480p rendering of an ATSC 1080i multiburst signal, 5 MHz<br />

is rescaled to 4.85 MHz, 10 MHz to 9.71, but 15 MHz, 20 MHz, 25 MHz, and<br />

30 MHz become any number of frequencies (including 12.44 MHz, 7.58 MHz,<br />

2.73 MHz, and 2.12 MHz respectively). These frequency aliases and respective<br />

amplitudes are measured and displayed in order: 2.12 MHz, 2.73 MHz,<br />

4.85 MHz, 7.58 MHz, 9.71 MHz, 12.44 MHz.<br />

How Results are<br />

Calculated<br />

The six largest peaks are found in the spectrum of signal on the pedestal. These<br />

frequencies are displayed in order from lowest to highest. For each of these<br />

frequencies, the maximum magnitude of the cross-correlation between the signal<br />

within the pedestal area and a windowed complex sinusoid is found. This gives<br />

the amplitude.<br />

Noise<br />

The unweighted noise within the nominal bandwidth of the video signal is<br />

measured to ensure that the video quality is not reduced by random errors such<br />

as those that cause ‘snow’.<br />

Signal Source<br />

You can use the matrix signal, or you can use any flat line or line pedestal signal.<br />

Interpreting Results<br />

As a rule of thumb, errors generally become visible when the signal-to-noise dB<br />

measurement ranges in the low 40s. However, the degree of visibility depends on<br />

many factors, including spectral distribution of the noise. In standard definition<br />

television, noise weighting filters such as the CCIR Recommendation (Rec)<br />

576 -2 unified weighting filter are used to weight the noise spectrum to better<br />

match the visibility of noise in typical viewing conditions. The unified weighting<br />

filter has been modified to exactly match the ‘visibility of noise characteristics’<br />

of 576 -2 on the screen for each selected video format.<br />

How Results are<br />

Calculated<br />

After line tilt and other low frequency distortions are removed from the signal,<br />

all AC signal content is spectrally weighted by the selected filter, if any, and the<br />

resulting RMS voltage is calculated along with the signal-to-noise ratio in dB<br />

using a 700 mV peak signal value.<br />

3-34 VM5000 Automatic Video Measurement Set <strong>User</strong> <strong>Manual</strong>

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