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ADL5310ACP-R2 数据表(PDF) 14 Page - Analog Devices |
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ADL5310ACP-R2 数据表(HTML) 14 Page - Analog Devices |
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14 / 20 page ![]() ADL5310 Rev. A | Page 14 of 20 The optional capacitor from LOG1 (LOG2) to ground forms a single-pole, low-pass filter in combination with the 5 kΩ resis- tance at this pin. For example, when using a CFLT of 10 nF, the 3 dB corner frequency is 3.2 kHz. Such filtering is useful in minimizing the output noise, particularly when IPD is small. Multipole filters are more effective in reducing the total noise; examples are provided in the AD8304 data sheet. Because the basic scaling at LOG1 (LOG2) is 0.2 V/decade, and thus a 4 V swing at the buffer output would correspond to 20 decades, it is often useful to raise the slope to make better use of the rail-to-rail voltage range. For illustrative purposes, both channels in Figure 34 provide a 0.5 V/decade overall slope (25 mV/dB). Thus, using IREF = 3 μA, VLOG runs from 0.2 V at IPD = 3 nA to 1.4 V at IPD = 3 mA; the buffer output runs from 0.5 V to 3.5 V, corresponding to a dynamic range of 120 dB (electrical, that is, 60 dB optical power). Further information on adjusting the slope and intercept, using a negative supply, and additional operations can be found in the AD8305 data sheet. CALIBRATION Each channel of the ADL5310 has a nominal slope and intercept at LOG1 (LOG2) of 200 mV/decade and 300 pA, respectively, when configured as shown in Figure 34. These values are untrimmed and the slope alone may vary by as much as 7.5% over temperature. For this reason, it is recommended that a simple calibration be done to achieve increased accuracy. While the ADL5310 offers improved slope and intercept matching compared to a randomly selected pair of AD8305 log amps, the specified accuracy can only be achieved by calibrating each channel individually. 1.0 1.2 1.4 0.8 0.6 0.4 0.2 0 2 3 4 1 0 –1 –2 –3 10n 100n 1 µ 10 µ 100 µ 1m 10m 1n IPD (A) CALIBRATED ERROR MEASURED OUTPUT IDEAL OUTPUT UNCALIBRATED ERROR Figure 35. Using 2-Point Calibration to Increase Measurement Accuracy Figure 35 shows the improvement in accuracy when using a 2- point calibration method. To perform this calibration, apply two known currents, I1 and I2, in the linear operating range between 10 nA and 1 mA. Measure the resulting output, V1 and V2, respectively, and calculate the slope m and the intercept b: m = (V1 – V2)/[log10(I1) – log10(I2)] (7) b = V1 – m × log10(I1) (8) The same calibration could be performed with two known optical powers, P1 and P2. This allows for calibration of the entire measurement system while providing a simplified relationship between the incident optical power and VLOG voltage: m = (V1 – V2)/(P1 – P2) (9) b = V1 – m × P1 (10) The uncalibrated error line in Figure 35 was generated assum- ing that the slope of the measured output was 200 mV/decade when in fact it was actually 194 mV/decade. Correcting for this discrepancy decreased measurement error up to 3 dB. MINIMIZING CROSSTALK Combining two high-dynamic-range logarithmic converters in one IC carries potential pitfalls concerning channel-to-channel isolation. Special care must be taken in several areas to ensure acceptable crosstalk performance, particularly when one or both channels may operate at very low input currents. Fastidious sup- ply bypassing—also necessary for overall stability—and careful board layout are important first steps for minimizing crosstalk. While the shared bias circuitry improves channel-to-channel matching and reduces power consumption, it is also a source of crosstalk that must be mitigated. The VSUM pins, which are internally shorted, should be bypassed with at least 1 nF to ground, and 20 nF is recommended for operation at the lowest currents (<30 nA). VSUM is of particular importance because it acts as a reference voltage input for each input system, but without the bandwidth limitation at low currents that the primary inputs incur. Disturbances at the VSUM pin that are well within the bandwidth of the input are tracked by the loop and do not generate disturbances at the output (aside from the generally minor perturbation in reference currents caused by voltage variations at IRF1 and IRF2). For this reason, the pole frequency at VSUM, which has a 16 kΩ typical source resistance, should be set below the minimum input system bandwidth for the lowest input current to be encountered. Because the low frequency noise at VSUM is also tracked by the loop within its available bandwidth, this is also a criterion for reducing the noise contribution at the output from the thermal noise of the 16 kΩ source resistance at VSUM. |
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