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Non-Linear Phase Noise Mitigation over Systems using Constellation Shaping: Experimental Dataset
- Citation Author(s):
-
DarioPilori
DET, Politecnico di Torino, Torino, ItalyAntoninoNespolaLINKS Foundation, Torino, ItalyGabriellaBoscoDET, Politecnico di Torino, Torino, Italy - Submitted by:
- Dario Pilori
- Last updated:
- Tue, 05/17/2022 - 22:21
- DOI:
- 10.21227/nfkc-vf85
- Data Format:
- Link to Paper:
- Links:
- License:
- Creative Commons Attribution
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Abstract
This dataset contains the full set of experimental waveforms that were used to produce the article "Non-Linear Phase Noise Mitigation over Systems using Constellation Shaping", published in the Journal of Lightwave Technology with DOI: 10.1109/JLT.2019.2917308.
The dataset contains two files: PartIII_NZDSF.tar and PartIV_GS.tar, corresponding to part III and part IV of the paper. Each file contains: * Transmitted one-sample-per-symbol sequence, that is loaded into the DAC. * Intradyne back-to-back results. * Propagation results over the recirculating loop. All data has been captured with a 50 GS/s Tektronix oscilloscope, and symbol rate is 16 GBaud. Back-to back results are quoted as a function of noise power, i.e. attenuation of the ASE source used for noise loading. Loop results are quoted as a function of the per-channel optical power and recirculation number. Details on the experiment are available on the paper.
Dataset Files
Dataset on Part IV of the paper: Geometrical Shaping over SMF PartIV_GS.tar (7.01 GB)- Dataset on Part III of the paper: Probabilistic Shaping over NZDSF PartIII_NZDSF.tar (19.33 GB)
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