4.6 Article

Ultra-Wideband Free-Space Optical Phase Stabilization

期刊

IEEE COMMUNICATIONS LETTERS
卷 25, 期 5, 页码 1610-1614

出版社

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/LCOMM.2021.3053943

关键词

Optical noise; Adaptive optics; Optical feedback; Phase noise; Optical variables measurement; Optical mixing; Atmospheric measurements; Free-space optics; optical communications; phase stabilization; atmospheric propagation; wavelength division multiplexing

资金

  1. SmartSat Cooperative Research Centre - Australian Government's CRC Program [1-01]
  2. Australian Research Council's Centre of Excellence for Engineered Quantum Systems (EQUS) [CE170100009]
  3. Forrest Research Foundation Fellowship
  4. SmartSat Cooperative Research Centre Top-Up Scholarship
  5. Australian Government Research Training Program (RTP) Scholarship

向作者/读者索取更多资源

The study demonstrates a system capable of suppressing atmospheric turbulence to achieve phase stability in free-space optical (FSO) communications, laying the foundation for 40 Tbps ground-to-space FSO transmission.
Free-space optical (FSO) communications have the potential to revolutionize wireless communications due to the advantages of greater inherent security, high-directionality, high available bandwidth and small physical footprint. The effects of atmospheric turbulence currently limit the performance of FSO communications. In this letter, we demonstrate a system capable of indiscriminately suppressing the atmospheric phase noise encountered by independent optical signals spread over a range of 7.2 THz (encompassing the full optical C-Band), by actively phase stabilizing a primary optical signal at 193.1 THz (1553 nm). We show similar to 30 dB of indiscriminate phase stabilization over the full range, down to average phase noise at 10 Hz of -39.6 dBc Hz(-1) when using an acousto-optic modulator (AOM) as a Doppler actuator, and -39.9 dBc Hz(-1) when using a fiber-stretcher as group-delay actuator to provide the phase-stabilization system's feedback. We demonstrate that this suppression is limited by the noise of the independent optical signals, and that the expected achievable suppression is over 40 dB greater, reaching around -90 dB Hz(-1) at 10 Hz. We conclude that 40 Tbps ground-to-space FSO transmission would be made possible with the combination of our stabilization system and other demonstrated technologies.

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