Chinese Optics Letters, 2018, 16 (4): 040604, Published Online: Jul. 12, 2018  

SER estimation method for 56 GBaud PAM-4 transmission system

Author Affiliations
1 COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan
2 Department of Electronic and Information Engineering, The Hong Kong Polytechnic University, Hong Kong, China
3 National University of Sciences and Technology (NUST), Islamabad, Pakistan
Figures & Tables

Fig. 1. Simulation setup of 56 GBaud PAM-4 transmission system.

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Fig. 2. Contour plots at (a) 4.41dBm, (b) 5.06dBm, (c) 5.71dBm, (d) 6.36dBm, (e) 7.01dBm, and (f) 7.66dBm for 30 GHz. (g) Contour lines at Z=0 for different ROPs at 30 GHz.

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Fig. 3. Contour lines at Z=0 for different ROPs at (a) 18 GHz, (b) 19 GHz, (c) 20 GHz, and (d) 25 GHz.

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Fig. 4. (a) SER versus ROPs at different bandwidths. (b) Contour plot at 5.71dBm for 18, 19, 20, 25, and 30 GHz. (c) P versus ROPs for 18, 19, 20, 25, and 30 GHz. (d) P versus receiver bandwidths at 4.41, 5.06, 5.71, 6.36, and 7.01dBm.(e) Comparison among SERC, SERQ, and SERGGD as a function of ROPs at 30 GHz. (f) SER verus P for 18, 19, 20, 25, and 30 GHz at 10 km.

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Fig. 5. (a) Eye-diagram and (b) probability distribution function of the received signal of PAM-4 at 7.66dBm at 30 GHz.

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Fig. 6. Experimental setup of 56 Gbaud PAM-4 transmission system.

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Fig. 7. Contour lines at Z=0 for 4, 5, 6, 7. (a) BtB. (b) 10 km. (c) SER versus ROPs for BtB and 10 km. (d) P versus ROPs at BtB and 10 km. (e) SER versus P at BtB and 10 km.

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Fig. 8. (a) Eye-diagram and (b) probability distribution function of the received signal of PAM-4 at 7dBm at 10 km.

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Table1. Simulation Parameters

ParameterValues
Length (km)10
Wavelength (nm)1310
Linewidth (MHz)5
Rx. BW (GHz)18,19,20,25, and 30
Power (dBm)0
PD thermal noise (pA/Hz0.5)20
PD dark current (nA)10
PD responsivity (A/W)1

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Aadil Raza, Kangping Zhong, Salman Ghafoor, Saeed Iqbal, Muhammad Adeel, Shahid Habib, Muhammad Fasih Uddin Butt, Chao Lu. SER estimation method for 56 GBaud PAM-4 transmission system[J]. Chinese Optics Letters, 2018, 16(4): 040604.

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