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Agilent Spectrum Analysis Basics - Agilent Technologies

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Noise figure<br />

Many receiver manufacturers specify the performance of their receivers in<br />

terms of noise figure, rather than sensitivity. As we shall see, the two can<br />

be equated. A spectrum analyzer is a receiver, and we shall examine noise<br />

figure on the basis of a sinusoidal input.<br />

Noise figure can be defined as the degradation of signal-to-noise ratio as a<br />

signal passes through a device, a spectrum analyzer in our case. We can<br />

express noise figure as:<br />

F = S i /N i<br />

S o /N o<br />

where<br />

F= noise figure as power ratio (also known as noise factor)<br />

S i = input signal power<br />

N i = true input noise power<br />

S o = output signal power<br />

N o = output noise power<br />

If we examine this expression, we can simplify it for our spectrum analyzer.<br />

First of all, the output signal is the input signal times the gain of the analyzer.<br />

Second, the gain of our analyzer is unity because the signal level at the<br />

output (indicated on the display) is the same as the level at the input<br />

(input connector). So our expression, after substitution, cancellation,<br />

and rearrangement, becomes:<br />

F = N o /N i<br />

This expression tells us that all we need to do to determine the noise figure<br />

is compare the noise level as read on the display to the true (not the effective)<br />

noise level at the input connector. Noise figure is usually expressed in terms<br />

of dB, or:<br />

NF = 10 log(F) = 10 log(N o ) – 10 log(N i ).<br />

We use the true noise level at the input, rather than the effective noise level,<br />

because our input signal-to-noise ratio was based on the true noise. As we<br />

saw earlier, when the input is terminated in 50 ohms, the kTB noise level at<br />

room temperature in a 1 Hz bandwidth is –174 dBm.<br />

We know that the displayed level of noise on the analyzer changes with<br />

bandwidth. So all we need to do to determine the noise figure of our<br />

spectrum analyzer is to measure the noise power in some bandwidth,<br />

calculate the noise power that we would have measured in a 1 Hz bandwidth<br />

using 10 log(BW 2 /BW 1 ), and compare that to –174 dBm.<br />

For example, if we measured –110 dBm in a 10 kHz resolution bandwidth,<br />

we would get:<br />

NF =<br />

[measured noise in dBm] – 10 log(RBW/1) – kTB B=1 Hz<br />

–110 dBm –10 log(10,000/1) – (–174 dBm)<br />

–110 – 40 + 174<br />

24 dB<br />

4. This may not always be precisely true for a given<br />

analyzer because of the way resolution bandwidth<br />

filter sections and gain are distributed in the IF chain.<br />

Noise figure is independent of bandwidth 4 . Had we selected a different<br />

resolution bandwidth, our results would have been exactly the same.<br />

For example, had we chosen a 1 kHz resolution bandwidth, the measured<br />

noise would have been –120 dBm and 10 log(RBW/1) would have been 30.<br />

Combining all terms would have given –120 – 30 + 174 = 24 dB, the same<br />

noise figure as above.<br />

61

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