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Optimal power split ratio for autobalanced photodetection

机译:自动平衡光电检测的最佳功率分配比

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摘要

The noise suppression of the autobalanced photoreceiver devised by Hobbs [Proc. SPIE 1376, 216 (1990)] had been determined to depend on the photocurrent ratio of reference beam to signal beam under the condition of constant signal beam photocurrent, and the best noise cancellation was suggested at a ratio close to 2. But in most applications, the available optical power has a limit. Therefore, to optimize the sensitivity of measurements, we should consider how to allocate the beam power in the case of fixed total optical power. In this paper, we measure the air Faraday rotation at different azimuth angles of beam polarization, which correspond to different photocurrent ratios. The signal-to-noise ratio at each photocurrent ratio is determined, and the best sensitivity appears at the photocurrent ratio of 1. This best sensitivity achieved is 3.02 × 10~(-8) rad Hz~(-1/2), which is about 1.3 times the shot noise limit. Our results are useful for sensitive optical measurements with the autobalanced photoreceiver.
机译:霍布斯设计的自动平衡光接收机的噪声抑制SPIE 1376,216(1990)]被确定为在恒定信号束光电流的条件下取决于参考束与信号束的光电流比,并且建议最佳的噪声消除比应接近2。但是在大多数应用中,可用光功率有限制。因此,为了优化测量的灵敏度,在总光功率固定的情况下,应考虑如何分配光束功率。在本文中,我们在不同的光束偏振方位角下测量了空气法拉第旋转,这对应于不同的光电流比。确定每个光电流比下的信噪比,并在光电流比为1时出现最佳灵敏度。此最佳灵敏度为3.02×10〜(-8)rad Hz〜(-1/2),其中约为散粒噪声极限的1.3倍。我们的结果对于使用自动平衡光接收器进行灵敏的光学测量非常有用。

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