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OPA692 Datasheet(PDF) 23 Page - Burr-Brown (TI) |
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OPA692 Datasheet(HTML) 23 Page - Burr-Brown (TI) |
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23 / 31 page ![]() www.ti.com GAIN ACCURACY AND LINEARITY 0.0200 0.0175 0.0150 0.0125 0.0100 0.0075 0.0050 0.0025 0 V (peak-to-peak) O 2 3 4 5 6 7 8 Figure42TestCircuit R =100W L R =500W L NOISE PERFORMANCE 700 600 500 400 300 200 100 0 Gain(V/V) Mean=1.9883 =0.0967 s 4kT R G R G R F R S 1/3 OPA3693 I BI E O I BN 4kT=1.6E 20J - at290K E RS E NI 4kTR S 4kTR F OPA3693 SBOS353 – DECEMBER 2006 much more voltage-swing-dependent on output distortion than strictly power-dependent. To use the 500 Ω intercept curve, use the single-tone voltage swing as if it were driving a 50 Ω load to compute the PO used in the intercept equation. The OPA3693 provides improved absolute gain accuracy and dc linearity over earlier fixed gain of two line drivers. Operating at a gain of +2V/V by tying the –IN pin to ground, the OPA3693 shows a maximum gain error of ±1% at +25°C. The dc gain therefore lies between 1.98V/V and 2.02V/V at room temperature. Over the specified temperature ranges, this gain tolerance expands only slightly due to the Figure 56. DC Linearity vs Output Swing and matched temperature drift for RF and RG. Achieving Loads this gain accuracy requires a very low impedance ground at –IN. Typical production lots show a much tighter distribution in gain than this ±1% specification. Figure 55 shows a typical distribution in measured gain at the gain of +2V/V configuration, in this case The OPA3693 offers an excellent balance between showing a slight drop in the mean (0.25%) from the voltage and current noise terms to achieve a low nominal but with a very tight distribution. output noise under a variety of operating conditions. The inverting node noise current (internal) appears at the output multiplied by the relatively low 300 Ω feedback resistor. The input noise voltage (1.8nV/ √Hz) is extremely low for a unity-gain stable amplifier. This low input voltage noise was achieved at the price of higher noninverting input current noise (17.8pA/ √Hz). As long as the ac source impedance looking out of the noninverting input is less than 100 Ω, this current noise does not contribute significantly to the total output noise. The op amp input voltage noise and the two input current noise terms combine to give low output noise for the each of the three gain settings available using the OPA3693. Figure 57 shows the op amp noise analysis model with all of the noise terms included. In this model, all noise terms are taken to be noise voltage or current density terms in either nV/ √Hz or pA/ √Hz. Figure 55. Typical +2V/V Gain Distribution The exceptionally linear output stage (as illustrated by the high 3rd-order intermodulation intercept) and low thermal gradient induced errors for the OPA3693 give an extremely linear output over large voltage swings and heavy loads. Figure 56 shows the tested deviation (in % of peak-to-peak) from linearity for a range of symmetrical output swings and loads. Below 4VPP, for either a 100Ω or a 500Ω load, the OPA3693 delivers greater than 14-bit linear output response. Figure 57. Op Amp Noise Model 23 Submit Documentation Feedback |
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