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AD9260EB Datasheet(PDF) 22 Page - Analog Devices |
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AD9260EB Datasheet(HTML) 22 Page - Analog Devices |
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22 / 36 page ![]() AD9260 –22– REV. B where q1 and q2 are the individual charges stored on capacitors CS1 and CS2 respectively, and CS is the capacitance value of CS1 and CS2. When capacitors CS1 and CS2 are connected to the Analog Modulator during the preceding “precharge” clock phase, the capacitors are precharged equal to an approximation of a previous sample of the input signal. Consequently the differential charge on these capacitors while CLK is high is given in the following equation, Q(n–1) = CS × VCORE(delay) + CS × Vdelta (7) where VCORE(delay) is the value of VCORE sampled during a previous period of CLK, and Vdelta is the sigma-delta error voltage left on the capacitors. Vdelta is a natural artifact of the sigma-delta feedback techniques utilized in the Analog Modula- tor of the AD9260. It is a small random voltage term that changes every clock period and varies from 0 to ±0.05 × VREF. The analog circuitry used to drive the input pins of the AD9260 must respond to the charge glitch that occurs when capacitors CS1 and CS2 are connected to input pins VINA and VINB. This circuitry must provide additional charge, qdelta, to capacitors CS1 and CS2, which is the difference between the precharged value, Q(n–1), and the new value, Q(n), as given in the follow- ing equation, Qdelta = Q(n) – Q(n–1) (8) Qdelta = CS × [VCORE–VCORE(delay) + Vdelta] (9) DRIVING THE INPUT Transient Response The charge glitch occurs once at the beginning of every period of the input CLK (falling edge), and the sample is taken on capacitors CS1 and CS2 exactly one-half period later (rising edge). Figure 56 presents a typical input waveform applied to input Pins VINA and VINB of the AD9260. CLOCK VINA-VINB TRACK SAMPLE TRACK SAMPLE TRACK SAMPLE TRACK SAMPLE Figure 56. Typical Input Waveform Figure 56 illustrates the effect of the charge glitch when a source with nonzero output impedance is used to drive the input pins. This source must be capable of settling from the charge glitch in one-half period of the CLK. Unfortunately, the MOS switches used in any CMOS-switched capacitor circuit (including those in the AD9260) include nonlinear parasitic junction capaci- tances connected to their terminals. Figure 55 also illustrates the parasitic capacitances, Cpa1, Cpb1, Cpa2 and Cpb2, associ- ated with the input switches. Parasitic capacitor Cpa1 and Cpa2 are always connected to Pins VINA and VINB and therefore do not contribute to the glitch energy. Parasitic capacitors Cpb1 and Cpb2, on the other hand, cause a charge glitch that adds to that of input capacitors CS1 and CS2 when they are connected to input Pins VINA and VINB. The nonlinear junction capacitance of Cpb1 and Cpb2 cause charge glitch energy that is nonlinearily related to the input signal. Therefore, linear settling is difficult to achieve unless the input source completely settles during one-half period of CLK. A portion of the glitch impulse energy “kicked” back at the source is not linearly related to the input signal. Therefore, the best way to ensure that the input signal settles linearly is to use wide bandwidth circuitry, which settles as completely as possible from the glitch during one-half period of the CLK. The AD9260 utilizes a proprietary clock-boosted boot-strapping technique to reduce the nonlinear parasitic capacitances of the internal CMOS switches. This technique improves the linearity of the input switches and reduces the nonlinear parasitic capaci- tance. Thus, this technique reduces the nonlinear glitch energy. The capacitance values for the input capacitors and parasitic capacitors for the input structure of the AD9260, as illustrated in Figure 55, are listed as follows. CS = 3.2 pF, Cpa = 6 pF, Cpb = 1 pF (where CS is the capaci- tance value of capacitors CS1 and CS2, Cpa is the value of capacitors Cpa1 and Cpa2, and Cpb is the value of capacitors Cpb1 and Cpb2). The total capacitance at each input pin is CIN = CS + Cpa + Cpb = 10.2 pF. Input Driver Considerations The optimum noise and distortion performance of the AD9260 can ONLY be achieved when the AD9260 is driven differentially with a 4 V input span . Since not all applications have a signal precon- ditioned for differential operation, there is often a need to per- form a single-ended-to-differential conversion. In the case of the AD9260, a single-ended-to-differential conversion is best realized using a differential op amp driver. Although a transformer will perform a similar function for ac signals, its usefulness is pre- cluded by its inability to directly drive the AD9260 and thus the additional requirement of an active low noise, low distortion buffer stage. Single-Ended-to-Differential Op Amp Driver There are two single-ended-to-differential op amp driver cir- cuits useful for driving the AD9260. The first circuit, shown in Figure 57, uses the AD8138 and represents the best choice in most applications. The AD8138 is a low-distortion differential ADC driver designed to convert a ground-referenced single- ended input signal to a differential output signal with a specified common-mode level for dc-coupling applications. It is capable of maintaining the typical THD and SFDR performance of the AD9260 with only a slight degradation in its noise performance in the 8 × mode (i.e., SNR of 85 dB–86 dB). In this application, the AD8138 is configured for unity gain and its common-mode output level is set to 2.5 V (i.e., VREF of the AD9260) to maximize its output headroom while operating from a single supply. Note, single-supply operation has the benefit of not requiring an input protection network for the AD9260 in dc-coupled applications. A simple R-C network at the output is used to filter out high-frequency noise from the AD8138. Recall, the AD9260’s small signal bandwidth is 75 MHz, hence any noise falling within the baseband bandwidth of the AD9260 defined by its sample and decimation rate, as well as “images” of its baseband response occurring at multiples of the sample rate, will degrade its overall noise performance. |
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