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LT6232IGN 数据表(PDF) 24 Page - Linear Technology |
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LT6232IGN 数据表(HTML) 24 Page - Linear Technology |
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24 / 24 page ![]() LT6230/LT6230-10/ LT6231/LT6232 24 sn623012 623012fas Linear Technology Corporation 1630 McCarthy Blvd., Milpitas, CA 95035-7417 (408) 432-1900 q FAX: (408) 434-0507 q www.linear.com ©LINEAR TECHNOLOGY CORPORATION 2003 LT/TP 0304 1K REV A • PRINTED IN USA RELATED PARTS PART NUMBER DESCRIPTION COMMENTS LT1028 Single, Ultra Low Noise 50MHz Op Amp 0.85nV/ √Hz LT1677 Single, Low Noise Rail-to-Rail Amplifier 3V Operation, 2.5mA, 4.5nV/ √Hz, 60µV Max VOS LT1806/LT1807 Single/Dual, Low Noise 325MHz Rail-to-Rail Amplifier 2.5V Operation, 550 µV Max VOS, 3.5nV/√Hz LT6200/LT6201 Single/Dual, Low Noise 165MHz 0.95nV √Hz, Rail-to-Rail Input and Output LT6202/LT6203/LT6204 Single/Dual/Quad, Low Noise, Rail-to-Rail Amplifier 1.9nV/ √Hz, 3mA Max, 100MHz Gain Bandwidth Photodiode Amplifier Time Domain Response Low Power Avalanche Photodiode Transimpedance Amplifier IS = 3.3mA 50ns/DIV 623012 TA02b + – R1 1.5k R2 1.5k C2 0.1 µF 5V –5V ENABLE LT6230 ≈ 200V BIAS ADVANCED PHOTONIX 012-70-62-541 WWW.ADVANCEDPHOTONIX.COM 623012 TA02a C1 4.7pF OUTPUT OFFSET = 500 µV TYPICAL BANDWIDTH = 20MHz OUTPUT NOISE = 1.1mVP–P (100MHz MEASUREMENT BW) TYPICAL APPLICATIO S The LT6230 is applied as a transimpedance amplifier with an I-to-V conversion gain of 1.5k Ω set by R1. The LT6230 is ideally suited to this application because of its low input offset voltage and current, and its low noise. This is be- cause the 1.5k resistor has an inherent thermal noise of 5nV/ √Hz or 3.4pA/√Hz at room temperature, while the LT6230 contributes only 1.1nV and 2.4pA / √Hz. So, with respect to both voltage and current noises, the LT6230 is actually quieter than the gain resistor. The circuit uses an avalanche photodiode with the cathode biased to approximately 200V. When light is incident on the photodiode, it induces a current IPD which flows into the amplifier circuit. The amplifier output falls negative to maintain balance at its inputs. The transfer function is therefore VOUT = –IPD • 1.5k. C1 ensures stability and good settling characteristics. Output offset was measured at 280 µV, so low in part because R2 serves to cancel the DC effects of bias current. Output noise was measured at 1.1mVP–P on a 100MHz measurement bandwidth, with C2 shunting R2’s thermal noise. As shown in the scope photo, the rise time is 17ns, indicating a signal bandwidth of 20MHz. |
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