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AD9042ST/PCB 数据表(PDF) 22 Page - Analog Devices |
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AD9042ST/PCB 数据表(HTML) 22 Page - Analog Devices |
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22 / 24 page ![]() AD9042 –22– REV. A AD9042 NOISE SOURCE (REF. FIGURE 53) LPF FROM RF/IF AIN VOFFSET VREF Figure 54. Using the AD9042 with Dither Receiver Example To determine how the ADC performance relates to overall receiver sensitivity, the simple receiver in Figure 55 will be examined. This example assumes that the overall down conversion process can be grouped into one set of specifications, instead of individually examining all components within the system and summing them together. Although a more detailed analysis should be employed in a real design, this model will provide a good approximation. In examining a wideband digital receiver, several considerations must be applied. Although other specifications are important, receiver sensitivity determines the absolute limits of a radio excluding the effects of other outside influences. Assuming that receiver sensitivity is limited by noise and not adjacent signal strength, several sources of noise can be identified and their overall contribution to receiver sensitivity calculated. RF/IF AD9042 CHANNELIZER REF IN DSP ENC 40.96MHz GAIN = 30dB NF = 20dB BW =12.5MHz SINGLE CHANNEL BW = 30kHz Figure 55. Receiver Analysis The first noise calculation to make is based on the signal band- width at the antenna. In a typical broadband cellular receiver, the IF bandwidth is 12.5 MHz. Given that the power of noise in a given bandwidth is defined by Pn = kTB, where B is bandwidth, k = 1.38 × 10–23 is Boltzman’s constant and T = 300k is absolute temperature, this gives an input noise power of 5.18 × 10–14 watts or –102.86 dBm. If our receiver front end has a gain of 30 dB and a noise figure of 20 dB, then the total noise presented to the ADC input becomes –52.86 dBm (–102.86 + 30 + 20) or 0.51 mV rms. Comparing receiver noise to dither required for good SFDR, we see that in this example, our receiver supplies about 10% of the dither required for good SFDR. Based on a typical ADC SNR specification of 68 dB, the equivalent internal converter noise is 0.140 mV rms. Therefore total broadband noise is 0.529 mV rms. Before processing gain, this is an equivalent SNR (with respect to full scale) of 56.5 dB. Assuming a 30 kHz AMPS signal and a sample rate of 40.96 MSPS, the SNR through processing gain is increased by 28.3 dB to 84.8 dB. However, if 8 strong and equal signals are present in the ADC bandwidth, then each must be placed 18 dB below full scale to prevent ADC overdrive. In addition, 3 dB to 15 dB should be used for ADC headroom should another signal come in-band unexpectedly. For this example, 12 dB of headroom will be allocated. Therefore we give away 30 dB of range and reduce the carrier-to-noise ratio (C/N)* to 54.8 dB. Assuming that the C/N ratio must be 6 dB or better for accurate demodulation, one of the eight signals may be reduced by 48.8 dB before demodulation becomes unreliable. At this point, the input signal power would be 40.6 µV rms on the ADC input or –74.8 dBm. Referenced to the antenna, this is –104.8 dBm. To improve sensitivity, several things can be done. First, the noise figure of the receiver can be reduced. Since front end noise dominates the 0.529 mV rms, each dB reduction in noise figure translates to an additional dB of sensitivity. Second, pro- viding broadband AGC can improve sensitivity by the range of the AGC. However, the AGC would only provide useful im- provements if all in-band signals are kept to an absolute minimal power level so that AGC can be kept near the maximum gain. This noise limited example does not adequately demonstrate the true limitations in a wideband receiver. Other limitations such as SFDR are more restrictive than SNR and noise. Assume that the analog-to-digital converter has an SFDR specification of –80 dBFS or –76 dBm (Full scale = +4 dBm). Also assume that a tolerable carrier-to-interferer (C/I)** (different from C/N) ratio is 18 dB. This means that the minimum signal level is –62 dBFS (–80 plus 18) or –58 dBm. At the antenna, this is –88 dBm. Therefore, as can be seen, SFDR (single or multi- tone) would limit receiver performance in this example. However, as shown previously, SFDR can be greatly improved through the use of dither (Figures 22, 25). In many cases, the addition of the out-of-band dither can improve receiver sensitivity nearly to that limited by thermal noise. Multitone Performance The plot below shows the AD9042 in a worst case scenario of four strong tones spaced fairly close together. In this plot no dither was used, and the converter still maintained 85 dBFS of spurious-free range. As illustrated previously, a modest amount of dither introduced out-of-band could be used to lower the nonlinear components. FREQUENCY – MHz 0 –80 –120 –40 –100 –20 –60 dc 20.5 4.1 8.2 12.3 16.4 ENCODE = 41 MSPS 3 6 9 7 4 258 Figure 56. Multitone Performance **C/N is the ratio of signal to inband noise. **C/I is the ratio of signal to inband interferer. |
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