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Data underpinning "Enhancing the Vertical Resolution of Coherent Optical Receivers"

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DataCite Commons2026-03-12 更新2026-05-07 收录
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https://rdr.ucl.ac.uk/articles/dataset/Data_underpinning_Enhancing_the_Vertical_Resolution_of_Coherent_Optical_Receivers_/24211254
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Data points for figures in the research paper "Enhancing the Vertical Resolution of Coherent Optical Receivers". Data can be visualised using software that can handle ".xlsx" files.1) The following files provide results obtained with a conventional coherent receiver and coherent receivers implementing optical intensity reshaping. All results were obtained in back-to-back configuration with noise loading. They allow reproducing Fig. 6:qfactor_vs_enob_b2b.xlsx: Q-factor vs effective number of bits (ENOB)qfactor_vs_jitter_b2b.xlsx: Q-factor vs RMS jitterqfactor_vs_skew_b2b.xlsx: Q-factor vs skewqfactor_vs_laser_lw_b2b.xlsx: Q-factor vs laser linewidthccdf_vs_skew_0ps_b2b_oir.xlsx, ccdf_vs_skew_0ps_b2b_conv.xlsx, ccdf_vs_skew_10ps_b2b_oir.xlsx &amp; ccdf_vs_skew_1ps_b2b_oir.xlsx: Complementary cumulative distribution function of peak-to-average power ratio at the presence of different skew values2) The following files provide results obtained with a conventional coherent receiver and coherent receivers implementing optical intensity reshaping. All results were obtained in WDM configuration, assuming a span length of 20 km. They allow reproducing Fig. 7:qfactor_vs_launchpower_oir_nodbp.xlsx &amp; qfactor_vs_launchpower_conv_nodbp.xlsx: Q-factor as a function of launch power for receivers implementing the technique of optical intensity reshaping and a conventional coherent receiver. Results without digital backpropagation.qfactor_vs_launchpower_oir_dbp.xlsx &amp; qfactor_vs_launchpower_conv_dbp.xlsx: Q-factor as a function of launch power for receivers implementing the technique of optical intensity reshaping and a conventional coherent receiver. Results with digital backpropagation.qfactor_vs_jitter.xlsx: Q-factor vs RMS jitter for the WDM scenarioqfactor_vs_skew: Q-factor vs skew for the WDM scenarioccdf_conv_jitter.xlsx, ccdf_oir_jitter.xlsx &amp; ccdf_oir_ops_jitter.xlsx: Complementary cumulative distribution function of peak-to-average power ratio at the presence of different RMS jitter values.ccdf_conv_skew.xlsx, ccdf_oir_skew.xlsx &amp; ccdf_oir_ops_skew.xlsx: Complementary cumulative distribution function of peak-to-average power ratio at the presence of different skew values.<br><br><br>

本数据集用于复现研究论文《增强相干光接收机的垂直分辨率》(Enhancing the Vertical Resolution of Coherent Optical Receivers)中的各类图表数据,可通过支持.xlsx格式文件的软件对数据集内容进行可视化展示。1) 以下文件包含传统相干光接收机与采用光强度整形技术的相干光接收机的测试结果,所有测试均在背靠背(back-to-back)配置且带噪声加载的条件下完成,可用于复现图6:qfactor_vs_enob_b2b.xlsx:Q因子与有效比特位数(ENOB,Effective Number of Bits)的对应关系;qfactor_vs_jitter_b2b.xlsx:Q因子与均方根(RMS,Root Mean Square)抖动的对应关系;qfactor_vs_skew_b2b.xlsx:Q因子与偏斜(skew)的对应关系;qfactor_vs_laser_lw_b2b.xlsx:Q因子与激光线宽的对应关系;ccdf_vs_skew_0ps_b2b_oir.xlsx、ccdf_vs_skew_0ps_b2b_conv.xlsx、ccdf_vs_skew_10ps_b2b_oir.xlsx 与 ccdf_vs_skew_1ps_b2b_oir.xlsx:不同偏斜值下峰均功率比的互补累积分布函数(CCDF,Complementary Cumulative Distribution Function)数据。2) 以下文件包含传统相干光接收机与采用光强度整形技术的相干光接收机的测试结果,所有测试均在波分复用(WDM,Wavelength Division Multiplexing)配置、跨距长度为20km的条件下完成,可用于复现图7:qfactor_vs_launchpower_oir_nodbp.xlsx 与 qfactor_vs_launchpower_conv_nodbp.xlsx:采用光强度整形技术的接收机与传统相干光接收机的Q因子随发射功率变化的曲线数据(未使用数字反向传播(DBP,Digital Backpropagation)技术);qfactor_vs_launchpower_oir_dbp.xlsx 与 qfactor_vs_launchpower_conv_dbp.xlsx:采用光强度整形技术的接收机与传统相干光接收机的Q因子随发射功率变化的曲线数据(已使用数字反向传播技术);qfactor_vs_jitter.xlsx:波分复用场景下Q因子与均方根抖动的对应关系数据;qfactor_vs_skew:波分复用场景下Q因子与偏斜的对应关系数据;ccdf_conv_jitter.xlsx、ccdf_oir_jitter.xlsx 与 ccdf_oir_ops_jitter.xlsx:不同均方根抖动值下峰均功率比的互补累积分布函数数据;ccdf_conv_skew.xlsx、ccdf_oir_skew.xlsx 与 ccdf_oir_ops_skew.xlsx:不同偏斜值下峰均功率比的互补累积分布函数数据。
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University College London
创建时间:
2023-09-28
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