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Agilent Spectrum Analysis Basics - Agilent Technologies

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Another specification is listed for the resolution filters: bandwidth selectivity<br />

(or selectivity or shape factor). Bandwidth selectivity helps determine the<br />

resolving power for unequal sinusoids. For <strong>Agilent</strong> analyzers, bandwidth<br />

selectivity is generally specified as the ratio of the 60 dB bandwidth to the<br />

3 dB bandwidth, as shown in Figure 2-9. The analog filters in <strong>Agilent</strong> analyzers<br />

are a four-pole, synchronously-tuned design, with a nearly Gaussian shape 4 .<br />

This type of filter exhibits a bandwidth selectivity of about 12.7:1.<br />

3 dB<br />

60 dB<br />

Figure 2-9. Bandwidth selectivity, ratio of 60 dB to 3 dB bandwidths<br />

For example, what resolution bandwidth must we choose to resolve signals<br />

that differ by 4 kHz and 30 dB, assuming 12.7:1 bandwidth selectivity? Since<br />

we are concerned with rejection of the larger signal when the analyzer is<br />

tuned to the smaller signal, we need to consider not the full bandwidth, but<br />

the frequency difference from the filter center frequency to the skirt. To<br />

determine how far down the filter skirt is at a given offset, we use the<br />

following equation:<br />

Where<br />

H(∆f) = –10(N) log 10 [(∆f/f 0 ) 2 + 1]<br />

H(∆f) is the filter skirt rejection in dB<br />

N is the number of filter poles<br />

∆f is the frequency offset from the center in Hz, and<br />

RBW<br />

f 0 is given by<br />

2 √2 1/N –1<br />

For our example, N=4 and ∆f = 4000. Let’s begin by trying the 3 kHz RBW<br />

filter. First, we compute f 0 :<br />

3000<br />

f 0 =<br />

= 3448.44<br />

2 √2 1/4 –1<br />

Now we can determine the filter rejection at a 4 kHz offset:<br />

4. Some older spectrum analyzer models used five-pole<br />

filters for the narrowest resolution bandwidths to<br />

provide improved selectivity of about 10:1. Modern<br />

designs achieve even better bandwidth selectivity<br />

using digital IF filters.<br />

18<br />

H(4000) = –10(4) log 10 [(4000/3448.44) 2 + 1]<br />

= –14.8 dB<br />

This is not enough to allow us to see the smaller signal. Let’s determine H(∆f)<br />

again using a 1 kHz filter:<br />

1000<br />

f 0 =<br />

= 1149.48<br />

2 √2 1/4 –1

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