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ADL5310ACP-R2 数据表(PDF) 13 Page - Analog Devices |
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ADL5310ACP-R2 数据表(HTML) 13 Page - Analog Devices |
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13 / 20 page ![]() ADL5310 Rev. A | Page 13 of 20 APPLICATIONS TEMPERATURE COMPENSATION REFERENCE GENERATOR 451 Ω 14.2k Ω 80k Ω 665k Ω 665k Ω 20k Ω 1k Ω 1nF 1k Ω 1nF 2k Ω 4.7nF 2k Ω 4.7nF 1nF 6.69k Ω 12k Ω 8k Ω 8k Ω CFLT2 10 nF CFLT1 10 nF COMM COMM VREF VNEG COMM VREF VRDZ VPOS VNEG VSUM INP2 IRF2 2.5V 0.5V ILOG IRF2 IRF1 OUT2 SCL2 BIN2 LOG2 VBIAS TEMPERATURE COMPENSATION 451 Ω 14.2k Ω 6.69k Ω 12k Ω COMM 5V VNEG VSUM INP1 IRF1 ILOG OUT1 VOUT1 VOUT2 SCL1 BIN1 LOG1 VBIAS IPD1 IPD2 0.5log10( ) IPD2 1nA 0.5log10( ) IPD1 1nA Figure 34. Basic Connections for Fixed Intercept Use The ADL5310 is easy to use in optical supervisory systems and in similar situations where a wide-ranging current is to be converted to its logarithmic equivalent—that is, represented in decibel terms. Basic connections for measuring a single current at each input are shown in Figure 34, which also includes various nonessential components, as explained next. The 2 V difference in voltage between the VREF and Input Pins INP1 and INP2, in conjunction with the external 665 kΩ resis- tors RRF1 and RRF2, provides 3 µA reference currents IRF1 and IRF2 into Pins IRF1 and IRF2. Connecting VRDZ to VREF raises the voltage at LOG1 and LOG2 by 0.8 V, effectively lowering each intercept current IINTC by a factor of 104 to position it at 300 pA. A wide range of other values for IREF, from 3 nA to 3 mA, may be used. The effect of such changes is shown in Figure 5 and Figure 8. Any temperature variation in RRF1 (RRF2) must be taken into account when estimating the stability of the intercept. Also, the overall noise increases when using very low values of IRF1 (IRF2). In fixed-intercept applications there is little benefit in using a large reference current, because doing so only compresses the low-current-end of the dynamic range when operated from a single supply. The capacitor between VSUM and ground is strongly recommended to minimize the noise on this node, to reduce channel-to-channel crosstalk, and to help provide clean reference currents. In addition, each input and reference pin (INP1, INP2, IRF1, and IRF2) has a compensation network made up of a series resistor and capacitor. The junction capacitance of the photo- diode along with the network capacitance of the board artwork around the input system creates a pole that varies widely with input current. The RC network stabilizes the system by simul- taneously reducing this pole frequency and inserting a zero to compensate an additional pole inherent in the input system. In general, the 1 nF, 1 kΩ network handles almost any photodiode interface. In situations where larger active area photodiodes are used, or when long input traces are used, the capacitor value may need to be increased to ensure stability. Although the signal and reference input systems are similar, additional care is required to ensure stable operation of the reference inputs at temperature extremes across the full current range of IRF1 (IRF2). It is recommended that filter components of 4.7 nF and 2 kΩ should be used from Pin IRF1 (IRF2) to ground. Temperature- stable components should always be used in critical locations such as the compensation networks; Y5V-type chip capacitors are to be avoided due to their poor temperature stability. |
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