Turbulence Mitigation via Multi-Plane Light Conversion and Coherent Optical Combination on a 200 m and a 10 km Link

A. Billaud, Andrew Reeves, A. Orieux, Helawae Friew, F. Gomez, Stephane Bernard, T. Michel, D. Allioux, J. Poliak, R. M. Calvo, O. Pinel
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引用次数: 3

Abstract

Current LEO satellites are generating more and more data which needs to be brought back to Earth for processing and analysis. Robust optical communications links are compulsory to be able to follow this growing demand for high-speed downlink with targets ranging from 10Gbps to 1Tbps. Atmospheric turbulences compensation is a key element to achieve such throughput. Here we investigate the capacity of turbulence mitigation via the use of a MPLC followed by an active optical recombiner, also called Tilba-Atmo. The MPLC demultiplexes the incoming turbulent beam into a set of gaussians beams whose relative energy distribution and relative phase evolves according to turbulence fluctuations. These gaussians are then sent into an active system based on a photonic integrated chip where the channels are optically recombined two-by-two in separate Mach-Zehnder interferometers. An 8-HGmode MPLC was placed at the reception end of a free space optical link in C or L-band. Different configurations where tried such as different levels of turbulence. Two different link lengths were tested, a 200m link with a 20cm telescope and a 10 km link at the DLR with a 10cm telescope which is normally use for testing and developing adaptive optics solutions. The first link showed high level of phase degradation on the received beam whilst on the second link the main effect of atmospheric turbulence was scintillation inside the pupil. In both cases tip-tilt was compensated via an auxiliary system and was not implemented inside the Tilba-Atmo component. The results are focused on comparison of fading in CW condition and in OOK communication between an SMF channel and the Tilba-Atmo channel. As this first version Tilba-Atmo is contributing to optical losses and optical recombining might be limited by the control electronics, a numerical sum of the demultiplexed modes is also performed to determine the upper limits of such a system.
在200米和10公里链路上通过多平面光转换和相干光学组合减少湍流
目前的低轨道卫星正在产生越来越多的数据,这些数据需要带回地球进行处理和分析。为了满足对10Gbps到1Tbps的高速下行链路不断增长的需求,强大的光通信链路是必不可少的。大气湍流补偿是实现这一吞吐量的关键因素。在这里,我们研究了通过使用MPLC和主动光学重组器(也称为Tilba-Atmo)来缓解湍流的能力。MPLC将入射湍流光束分解成一组高斯光束,这些高斯光束的相对能量分布和相对相位随湍流波动而变化。然后将这些高斯信号发送到一个基于光子集成芯片的有源系统中,在该系统中,通道在单独的马赫-曾德尔干涉仪中进行二对二的光学重组。在C或l波段的自由空间光链路的接收端放置一个8-HGmode MPLC。我们尝试了不同的配置,比如不同程度的湍流。测试了两种不同长度的链路,一种是200米的链路,使用20厘米的望远镜,另一种是DLR的10公里链路,使用10厘米的望远镜,通常用于测试和开发自适应光学解决方案。第一个环节显示了接收光束的高度相位退化,而在第二个环节中,大气湍流的主要影响是瞳孔内部的闪烁。在这两种情况下,倾斜都是通过辅助系统补偿的,而不是在Tilba-Atmo组件内实现的。重点比较了SMF信道和Tilba-Atmo信道在连续波条件下和OOK通信条件下的衰落。由于第一个版本的Tilba-Atmo会造成光学损耗,并且光学重组可能受到控制电子器件的限制,因此还进行了解复用模式的数值求和,以确定这种系统的上限。
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