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ADL5506ACBZ-R7 数据表(PDF) 21 Page - Analog Devices |
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ADL5506ACBZ-R7 数据表(HTML) 21 Page - Analog Devices |
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21 / 24 page ![]() ADL5506 Data Sheet Rev. A | Page 20 of 23 Effect of Waveform Type on Intercept Although specified for input levels in decibels relative to 1 mW (dBm), the ADL5506 fundamentally responds to voltage and not to power. A direct consequence of this characteristic is that input signals of equal rms power but differing crest factors, produce different results at the output of the log amplifier. The effect of differing signal waveforms is to shift the effective value of the intercept upwards or downwards. Graphically, this looks like a vertical shift in the transfer function of the log amplifier. The logarithmic slope, however, is not affected. For example, consider the case of the ADL5506 being alternately fed by an unmodulated sine wave and by a 64 QAM signal of the same rms power. The output voltage of the ADL5506 differs by the equivalent of 1.6 dB (31 mV) over the complete dynamic range of the device (with the output for a 64 QAM input being lower). Figure 35 and Figure 38 shows the transfer function of the ADL5506 when driven by both an unmodulated sine wave and several different signal waveforms. For precision operation, calibrate the ADL5506 for each signal type that is driving it. To measure the rms power of a 64 QAM input, for example, add the millivolt equivalent of the decibel value of the intercept shift (18.5 mV/dB × 1.5 dB) to the output voltage of the ADL5506. Temperature Drift at High Frequencies Figure 23 and Figure 27 show the log slope and error over temperature for a 3.5 GHz and 4.5 GHz input signal, respectively. Error due to drift over temperature consistently remains within ±0.5 dB for a temperature range of 0°C to 85°C. Temperatures below 0°C begin to exhibit error beyond 0.5 dB with error becoming no worse than −3 dB typical at −40°C. For all frequencies using a reduced temperature range, higher measurement accuracy is achievable. Operation Above 4.5 GHz The ADL5506 works at high frequencies but exhibits slightly higher output voltage temperature drift, especially at cold temperatures as described in the Temperature Drift at High Frequencies section. Figure 49 and Figure 50 show VLOG vs. PIN over frequency from 30 MHz to 6 GHz. The ADL5506 exhibits a significant intercept shift, high power ripple, and a continued decrease of the slope, which all contribute to a decrease in dynamic range. The changes in performance that occur as frequency is increased is partly due to less energy transferring into the device and partly to the bandwidth limitation of the limiting amplifier stages. Figure 49. VLOG vs. PIN over Frequency (30 MHz to 4500 MHz) Figure 50. VLOG vs. PIN over Frequency (4.5 GHz to 6 GHz) 10 0 –10 –20 –30 –40 –50 1.1 1.0 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 0.1 PIN (dBm) 30MHz 50MHz 100MHz 450MHz 900MHz 1900MHz 2140MHz 2700MHz 3500MHz 4500MHz 10 0 –10 –20 –30 –40 –50 1.2 1.0 0.8 0.6 0.4 0 0.2 PIN (dBm) 4.5GHz 5GHz 5.5GHz 6GHz |
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