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AD8033 bảng dữ liệu(PDF) 18 Page - Analog Devices |
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AD8033 bảng dữ liệu(HTML) 18 Page - Analog Devices |
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18 / 20 page ![]() REV. B –18– AD8033/AD8034 Wideband Photodiode Preamp Figure 12 shows an I/V converter with an electrical model of a photodiode. The basic transfer function is V IR sC R OUT PHOTO F FF = × + 1 where IPHOTO is the output current of the photodiode, and the parallel combination of RF and CF sets the signal bandwidth. The stable bandwidth attainable with this preamp is a function of RF, the gain bandwidth product of the amplifier, and the total capacitance at the amplifier’s summing junction, including CS and the amplifier input capacitance. RF and the total capaci- tance produce a pole in the amplifier’s loop transmission that can result in peaking and instability. Adding CF creates a zero in the loop transmission that compensates for the pole’s effect and reduces the signal bandwidth. It can be shown that the signal bandwidth resulting in a 45 ° phase margin (f(45)) is defined by the expression f f RC CR FS () 45 2 = ×× π fCR is the amplifier crossover frequency. RF is the feedback resistor. CS is the total capacitance at the amplifier summing junction (amplifier + photodiode + board parasitics). The value of CF that produces f(45) can be shown to be C C Rf F S FCR = ×× 2 π The frequency response in this case will show about 2 dB of peaking and 15% overshoot. Doubling CF and cutting the bandwidth in half will result in a flat frequency response, with about 5% transient overshoot. The preamp’s output noise over frequency is shown in Figure 13. The pole in the loop transmission translates to a zero in the amplifier’s noise gain, leading to an amplification of the input voltage noise over frequency. The loop transmission zero introduced by CF limits the amplification. The noise gain’s bandwidth extends past the preamp signal bandwidth and is eventually rolled off by the decreasing loop gain of the amplifier. Keeping the input terminal impedances matched is recommended to eliminate common-mode noise peaking effects that will add to the output noise. Integrating the square of the output voltage noise spectral density over frequency and then taking the square root results in the total rms output noise of the preamp. CS RSH = 10 11 VB IPHOTO RF CF VO CM RF CM CD CF + CS Figure 12. Wideband Photodiode Preamp FREQUENCY – Hz 2 RFCF 2 RF (CF + CS + CM + 2CD) (CS + CM + 2CD + CF) /CF RF NOISE VEN (CF + CS + CM + 2CD) /CF f3 f2 f3 = VEN f1 f2 = f1 = 1 1 fCR NOISE DUE TO AMPLIFIER Figure 13. Photodiode Voltage Noise Contributions |
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