A detection technique for high order QAM in the presence of transmitter angular skew

Sawitree Wongroekdee, V. Imtawil, Puripong Suthisopapan
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Abstract

Angular skew arising from imperfect biasing of the transmitter can cause a significant performance degradation in high speed optical QAM systems. A simple approach to detect QAM signal under the effect of angular skew is Gram-Schmidt orthogonalization procedure (GSOP). However, this approach has poor performance when the size of QAM constellation exceeds 256. To solve this problem, a new detection algorithm is proposed. From the results, the proposed technique outperforms the GSOP. It provides the skew tolerance of up to 25-degrees at BER of 10-5 for the expense of 1 dB Eb/No penalty.
一种高阶QAM在发射机角倾斜情况下的检测技术
在高速光学QAM系统中,由发射机不完全偏置引起的角倾斜会导致性能的显著下降。Gram-Schmidt正交化法(GSOP)是一种检测角偏斜影响下QAM信号的简单方法。但是,当QAM星座的大小超过256个时,这种方法的性能就会变差。为了解决这一问题,提出了一种新的检测算法。结果表明,该方法优于GSOP。在BER为10-5的情况下,它提供了高达25度的倾斜公差,而代价是1 dB Eb/无损失。
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