利用铋离子对 25 Gbaud 平衡光接收器进行辐射测试,以实现高达 70 MeV cm2/mg 的线性能量转移

Abhay M. Joshi, S. Datta, Abigale R. Joshi, Michael Sivertz, David Inzalaco, Joel Hatch
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摘要

从低地球轨道卫星通信星座到星际链路和深空任务等多个平台都需要采用高速光接收器(即与跨阻抗放大器(TIA)集成的光电二极管)的天基光通信链路。我们之前的研究已经证明,InP/InGaAs 光电二极管在受到各种离子照射时能够抵御辐射引起的位移和电离损伤。此外,还有必要对在高线性能量转移(LET)重离子辐照下可能会因单次事件效应(SEE)而出现闩锁(latch ups)的 TIA 进行鉴定。我们介绍了一种平衡砷化镓光接收器,即一对匹配的光电二极管和一个硅 CMOS TIA,它具有自动增益控制模式,支持相干和直接探测光通信链路,符号速率高达 25 Gbaud,总数据速率高达 100 Gbps 或更高。这些器件分别承受了 76 MeV/n、96 MeV/n 和 154 MeV/n 的铋离子,每种离子能量的通量为 1E7 离子/平方厘米。选择离子能量的目的是使 LET-Si 达到 ⪆70 MeV-cm2 /mg。在辐射运行期间,对 TIA 进行偏置,并连续记录其驱动电流和射频输出噪声频谱。辐照前后对这些器件进行的详细模拟和数字表征补充了原位数据,包括光电二极管暗电流、TIA 驱动电流、射频响应、射频回波损耗、噪声频谱、25 Gbps 幅度偏移键控(ASK)眼图和误码率,以及 10.709 Gbps 归零差分相移键控(RZ-DPSK)眼图和误码率。我们没有观察到辐射对这些设备造成任何重大影响。
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Radiation testing of 25 Gbaud balanced photoreceivers with bismuth ions for linear energy transfer up to 70 MeV cm2/mg
Space-based optical communication links incorporating high speed photoreceivers, i.e. photodiodes integrated with Transimpedance Amplifiers (TIA), are required for multiple platforms, from low earth orbit satellite communication constellations to inter-planetary links and deep space missions. Our prior studies have demonstrated that InP/InGaAs photodiodes are resilient to radiation induced displacement and ionization damage when irradiated with a wide variety of ions. It is also necessary to qualify TIAs that may exhibit latch ups due to Single Event Effect (SEE) when irradiated with heavy ions having high Linear Energy Transfer (LET). We present a balanced InGaAs photoreceiver, i.e. a matched pair of photodiodes followed by a Silicon CMOS TIA, with automatic gain control mode that supports coherent and direct detection optical communication links with a symbol rate up to 25 Gbaud and aggregate data rate up to 100 Gbps and beyond. These devices were subjected to 76 MeV/n, 96 MeV/n, and 154 MeV/n Bismuth Ions up to a fluence of 1E7 ions/cm2 for each ion energy. The ion energies were chosen with the objective of achieving LET-Si of ⪆70 MeV-cm2 /mg. During the radiation runs, the TIAs were biased and their drive currents and RF output noise spectra were continuously recorded. The in-situ data was complemented by detailed analog and digital characterization of these devices before and after irradiation, including photodiode dark current, TIA drive current, RF response, RF return loss, noise spectrum, 25 Gbps Amplitude Shift Keyed (ASK) eye diagrams and bit error ratio, and 10.709 Gbps Return to Zero Differential Phase Shift Keyed (RZ-DPSK) eye diagrams and bit error ratio. We did not observe any significant impact on these devices due to radiation.
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