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A Low-Power, Low-Noise 37-MHz Photoreceiver for Intersatellite Laser Interferometers Using Discrete Heterojunction Bipolar Transistors

机译:适用于使用离散异质结双极晶体管的星际激光干涉仪的低功耗,低噪声37MHz光接收器

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摘要

Intersatellite laser interferometers feature quadrant photoreceivers to produce electrical signals from the interfered optical beams. In the particular case of Laser Interferometer Space Antenna, the expected optical ac beat note has an amplitude of the order of nanowatts. This requires photoreceivers with an input current noise density of a fewn${mathrm {pA}} cdot {mathrm {Hz}}^{-1/2}$nin each channel up to 25 MHz. In addition, the significant number of photoreceivers in a single spacecraft imposes tight constraints on the power consumption per device. We present the experimental characterization of a quadrant photoreceiver based on discrete heterojunction bipolar transistors and an off-the-shelf 0.5-mm-diameter InGaAs quadrant photodiode, showing an input current noise density of 1.9n${mathrm {pA}} cdot {mathrm {Hz}}^{-1/2}$nat 25 MHz, a 3-dB bandwidth of 37 MHz, and a total power consumption of 178 mW.
机译:卫星间激光干涉仪具有象限光接收器,可以从受干扰的光束中产生电信号。在激光干涉仪空间天线的特定情况下,预期的光学交流拍频音的幅度约为纳瓦。这要求光接收器的输入电流噪声密度为n $ {mathrm {pA}} cdot {mathrm {Hz}} ^ {-1/2} $ 在每个通道中最多25 MHz。另外,单个航天器中大量的光接收器对每个设备的功耗施加了严格的约束。我们介绍了基于离散异质结双极晶体管和现成的0.5mm直径InGaAs象限光电二极管的象限光电接收器的实验特性,其输入电流噪声密度为1.9n $ {mathrm {pA }} cdot {mathrm {Hz}} ^ {-1/2} $ nat 25 MHz,3 dB带宽为37 MHz,总功耗为178 mW 。

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