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Agilent Spectrum Analysis Basics - Agilent Technologies

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External harmonic mixer<br />

Input<br />

signal<br />

Atten<br />

3 GHz<br />

3.9214 GHz<br />

321.4 MHz 21.4 MHz<br />

Analog or<br />

digital IF<br />

Input<br />

signal<br />

3 - 7 GHz<br />

3.6 GHz<br />

300 MHz<br />

Preselector<br />

321.4 MHz<br />

Sweep<br />

generator<br />

Display<br />

Figure 7-14. Block diagram of spectrum analyzer and external mixer with built-in preselector<br />

Signal identification<br />

Even when using an unpreselected mixer in a controlled situation, there<br />

are times when we must contend with unknown signals. In such cases, it is<br />

quite possible that the particular response we have tuned onto the display<br />

has been generated on an LO harmonic or mixing mode other than the one<br />

for which the display is calibrated. So our analyzer must have some way<br />

to tell us whether or not the display is calibrated for the signal response in<br />

question. For the purposes of this example, assume that we are using an<br />

<strong>Agilent</strong> 11970V 50 to 75 GHz unpreselected mixer, which uses the 14 – mixing<br />

mode. A portion of this millimeter band can be seen in Figure 7-15.<br />

The <strong>Agilent</strong> E4407B ESA-E spectrum analyzer offers two different<br />

identification methods: Image shift and Image suppress. We shall first<br />

consider the image shift method. Looking at Figure 7-16, let’s assume that<br />

we have tuned the analyzer to a frequency of 58.5 GHz. The 14 th harmonic<br />

of the LO produces a pair of responses, where the 14 – mixing product appears<br />

on screen at the correct frequency of 58.5 GHz, while the 14 + mixing product<br />

produces a response with an indicated frequency of 57.8572 GHz, which is<br />

2 times f IF below the real response. Since the ESA has an IF frequency of<br />

321.4 MHz, the pair of responses is separated by 642.8 MHz.<br />

98

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