International Journal of Networks and Communications
p-ISSN: 2168-4936 e-ISSN: 2168-4944
2019; 9(1): 37-52
doi:10.5923/j.ijnc.20190901.03

Mays M. Ibrahim, Raad S. Fyath
Department of Computer Engineering, Al-Nahrain University, Baghdad, Iraq
Correspondence to: Mays M. Ibrahim, Department of Computer Engineering, Al-Nahrain University, Baghdad, Iraq.
| Email: | ![]() |
Copyright © 2019 The Author(s). Published by Scientific & Academic Publishing.
This work is licensed under the Creative Commons Attribution International License (CC BY).
http://creativecommons.org/licenses/by/4.0/

This paper investigates the noise characteristics and transmission performance of Nyquist half-cycle single-sideband system incorporating amplified or unamplified optical link. The system design is based on intensity modulation/optical carrier assisted direct detection scheme. Digital signal processing is used at the receiver to compensate dispersion and nonlinearity of the optical fiber. Simulation results are presented for both 1310 and 1550 nm single-channels carrying 224 Gbps 16-QAM data. The results are used as a guideline to extend the results for O- and C-band wavelength division multiplexing (WDM) systems. The maximum transmission distance Lmax is deduced for different systems using a bit error rate threshold of 4.5×10-3 which corresponds to 7% overhead decision forward error correcting code. The results reveal that Lmax of the unamplified 1550 nm single-channel system is about 1.75 time that of the 1310 nm counterpart. The simulation is reversed when optical amplifiers are used to compensate fiber loss leading to higher transmission distance at 1310 nm. Further, using 0 dB carrier and signal lasers offer 44 and 72 km transmission distance for the unamplified 16-channel WDMs operating at O- and C-bands, respectively. Inserting optical amplifiers changes these values to 450 and 110 km, respectively. The simulation results are performance using Optisystem ver. 14 and are in good agreement with published experimental data.
Keywords: Nyquist half cycle (NHC) optical communication, O- and C-bands NHC, 16-QAM IM/DD, Optical SSB 16-QAM
Cite this paper: Mays M. Ibrahim, Raad S. Fyath, Performance Comparison between O- and C-bands Optical Carrier-Assisted Nyquist Half-Cycle SSB Communication Systems, International Journal of Networks and Communications, Vol. 9 No. 1, 2019, pp. 37-52. doi: 10.5923/j.ijnc.20190901.03.
symbol rate with zero ISI is equal to
. In other words, the raised-cosine filter shaping is redesigned here using approximated zero roll-off factor.(iii) Transmitting only one single-sideband (SSB) of the optical modulated carrier [25, 26-28]. The SSB transmission also reduces the effect of fiber group-velocity dispersion (GVD) which limits the maximum transmission distance in high-bit rate communication fiber link [29, 30].(iv) Using wavelength-division multiplexing (WDM) [9, 14, 22, 25, 31, 32] and polarization-division multiplexing (PDM) [11, 16, 27]. The PDM uses dual-polarization (DP) transmission to double the transmitted data rate.Recently, NHC-SSB SCM attracts increasing interest as a high spectral efficiency-modulation scheme suitable for high-bit rate links in short- and medium-reach optical network applications [1, 17, 25, 31]. An optical link based on this modulation scheme can be implemented using IM/DD configuration which reduces the cost and increases the robustness of the link. In 2017, Zhu et al. [23] have demonstrated the transmission of 16-QAM 224 Gbps data over 160 km standard single-mode fiber (SSMF) at C-band using NHC-SSB modulation. The transmission system uses optical carrier-assisted (OCA) technique to enhance the detection efficiency of the used DD receiver. In the experiment, the optical carrier was added with an additional (signal) laser at the transmitter side and the resultant waveform was delivered along the fiber. The scheme is equivalent to heterodyne coherent detection with a local oscillator and a single-ended photodiode (PD). The experimental results of Ref. [23] set a record of fiber link length for C-band 224 Gbps single channel and single PD direct detection transmission. Therefore, the OCA-NHC SSB configuration will be used as a basis for investigation in this work. The aim of is to investigate the transmission performance of NHC-SSB system operating at different link environments. This includes a single-channel and WDM systems operating at C- and O-bands with and without optical amplification using IM/DD scheme.![]() | (1a) |
![]() | (1b) |
is the symbol rate,
is the bit rate, and M is the modulation order.(iii) A high-order optical bandpass filter is used to select the lower-sideband (LSB) of the optical modulator output.(iv) The system uses two laser sources. A signal laser of frequency
which is modulated by the data. The second laser is called the carrier laser of frequency
and acts as an assisted carrier. The fields of the modulated signal laser and carrier laser should be combined before optical detection and therefore, the detection process is based on OCA-scheme. This scheme is useful for using DD receiver to detect the optical SSB signal.(v) The optical receiver uses a digital signal processing (DSP) unit for compensating fiber dispersion and nonlinear optics effects.(vi) The transmission link consists mainly of a SSMF. If optical amplifiers (OAs) are used to compensate fiber losses, the link is divided into many spans. Each span consists of 50 km SSMF followed by an OA to compensate the span loss.(vii) The field of the continuous-wave (CW) carrier laser can be combined with the field of the SSB component of the modulated signal laser at the transmitter side. This scheme is useful since both carrier and signals lasers are under control in the transmitter side. However, in WDM system, the carrier laser may be used in the receiver side to reduce the interference with near neighboring signal channels and also to reduce the effect of fiber nonlinear optics.![]() | (2) |
is the assisted optical carrier and
is the SSB optical signal. The polarization of both
and
are assumed to be aligned along the x axis with
denotes the unit vector of the x polarization. Further,![]() | (3a) |
![]() | (3b) |
Field amplitude of the CW optical carrier.
Frequency of the CW optical carrier.
Field amplitude of the CW optical signal.
Frequency of the CW optical signal.
frequency of the RF subcarrier.
Baseband signal with |u (t)|≤1.Assume that the optical channel has idea characteristics (i.e., the effect of attenuation, dispersion, and nonlinear optics are negligible) and the receiver performance is dominated by the contribution of amplified spontaneous emission (ASE) noise
generated by the in-line optical amplifiers![]() | (4) |
and
denote the ASE noise sources in both polarization and
is the unit vector of the y polarization. Under these assumptions, the received optical signal r(t) can be written as ![]() | (5a) |
![]() | (5b) |
and
are the x and y polarization components, respectively.![]() | (6a) |
![]() | (6b) |
which is related to the square of the incident field amplitude![]() | (7) |
is PD responsitivity with is PD quantum efficiency, q is the electron charge, h is Planck’s constan, t and
is the frequency of the incident field.Inserting eqns. (6a) and (6b) into eqn. (7) yields ![]() | (8) |
is the intermediate frequency
and Re [.] denotes the real part of the complex argument.To get a clear physical insight on eqn. (8), the photocurrent may splitted into group of components
Dc component.
Desired signal.
Signal-signal beat interference (SSBI).
Carrier-noise (from the same polarization) beating.
Signal-noise (from the same polarization) beating.
Noise-noise beating.The expressions of these six photocurrent component are as follows ![]() | (9a) |
![]() | (9b) |
![]() | (9c) |
![]() | (9d) |
![]() | (9e) |
![]() | (9f) |
can be deduced from the photocurrent ![]() | (10) |
and
are the average power of the signal and noise associated with the photocurrent, respectively.![]() | (11a) |
Here
denotes the expectation of the argument![]() | (11b) |
is the spectral density of the received ASE noise in each polarization and
is the optical band pass filter (OBPF) bandwidth used at the receiver side to suppress the amplified spontaneous emission noise incident on the PD.Substituting eqns. (11a) and (11b) into eqn. (10) gives![]() | (12) |
and the power of the optical signal
The carrier-to-signal power ratio is then given by ![]() | (13a) |
![]() | (13b) |
is reference optical bandwidth which is usually set to 0.1 nm in the measurement.(ii) After the photodetection, the signal-to-SSBI ratio SIR is given by![]() | (14) |
and
Then the electrical SNR can be rewritten as (see eqn. (12))![]() | (15) |
which is related to the square of the incident field amplitude![]() | (16) |
![]() | (17) |
![]() | (18) |
and
denote the direct-current (DC) component, desired signal, and SSBI, respectively, which are given by![]() | (19a) |
![]() | (19b) |
![]() | (19c) |
can be blocked by inserting a series capacitance in the current path.(ii) The signal component
represents a DSB/suppressed carrier (SC) as a modulated version of the baseband signal
with an effective RF carrier having a frequency equals
. Coherent (synchronous) quadrature demodulator should be used to recover the signal
from the component
.(iii) The SSBI component
cannot be eliminated by any filtering process since its spectrum overlaps with the signal spectrum.The electrical signal-to-noise ratio
associated with the photocurrent can be computed from eqn. (10). In the absence of optical amplification, the main receiver noise components are thermal noise, which is mainly due to the front-end electronic amplifier used to amplify the photogenerated current, carrier shot noise, and signal shot noise [32]![]() | (20a) |
, and
denote, respectively, the standard deviations (root-mean-square (RMS)) noise currents and they are given by![]() | (20b) |
![]() | (20c) |
![]() | (20d) |
load resistance and
noise figure [33]. In this equation,
is Boltzmann constant, T is the absolute temperature (in Kelvin), and
is the receiver electrical bandwidth. Equations (20c) and (20d) are deduced from the fact that the power spectral density (PSD) of the shot noise equals
average current), where q is the magnitude of the electric charge [34].The electrical SNR of the unamplified-link system is then given by ![]() | (21) |
and
denote, respectively, the carrier and signal power estimated at the end of the fiber link whose length is L, and they are related to the power launched at the fiber input
by![]() | (22a) |
![]() | (22b) |
(measured in
by![]() | (23) |
![]() | (24) |
the carrier laser field is coupled with the received signal field, and the resultant waveform is applied to the PD), then eqn. (24) can be modified to cover this case![]() | (25) |
is the power of the receiver-side inserted CW carrier laser. Here
is the electrical SNR corresponding to the case of an unamplified link supported with carrier laser inserted at the receiver side.
reported in this section correspond to the lengths of the fiber link which make the receiver bit error rate (BER) approaches its threshold value. A
BER threshold is used here which corresponds to 7% overhead hard-decision (HD) forward-error correcting (FEC). The simulation results are obtained using Optisystem ver. 14 software package.
dBm,
dBm (inserted at the transmitter side) and fiber length L =36 km. This link length corresponds to the maximum transmission distance,
, under these conditions. Note that the a double-side band (DSB) spectrum of the modulated radio frequency (RF) subcarrier covers approximately 56 GHz bandwidth which corresponds to
when
. This 56 GHz bandwidth also equals the bandwidth of the transmitted optical SSB signal. Note further, the ability of used DSP unit to compensate the fiber dispersion and recover the required constellation diagram. The simulation is repeated for the unamplified 1550 nm single-channel system (Scenario B1) and the results are reported in the Appendix. ![]() | Figure 2. Spectra and constellation diagrams related to an unamplified link 224 Gbps 16-QAM system operating at 1310 nm wavelength with L=36 km, Ps=0 dBm and Pc=0 dBm (carrier at transmitter). (a) Spectrum of the QAM pulse generator output (I-phase component). (b) Spectrum of the QAM modulator input. (c) Spectrum of the QAM modulator output. (d) Spectrum of the optical modulator output. (e) Spectrum of the optical SSB signal. (f) Spectrum of signal SSB + assisted carrier. (g) Spectrum of the optical signal at the fiber output. (h) Spectrum of the amplified photocurrent. (i) Spectrum of the QAM demodulator output. (j) Spectrum of the filtered QAM demodulator output. (k) Receiver constellation diagram at the DSP input. (L) Receiver constellation diagram at the DSP output |
is set to 0 dBm, and the values of
are estimated for different values of signal laser power 
![]() | Figure 3. Variation of maximum reach Lmax with signal laser power Ps assuming unamplified 224 Gbps 16-QAM system operating with Pc=0 dBm. (a) Carrier at the transmitter. (b) Carrier at the receiver |
![]() | Figure 4. Variation of maximum reach Lmax with signal laser power Ps assuming amplified 224 Gbps 16-QAM system operating with Pc=0 dBm. (a) Carrier at the transmitter. (b) Carrier at the receiver |
and carries 224 Gbps 16-QAM date rate per channel. The frequency of
channel laser is computer from
Figure 5 shows the spectrum of the O-band multiplexed signal at the fiber input and after 43 km transmission over unamplified link. The results are presented for
dBm,
dBm (inserted at the receiver side, L=Lmax=43 km, and N = 32). Note that the output spectrum is almost a copy of the input spectrum indicating the absence of distortion due to four-wave mixing (FWM) associated with fiber nonlinear optics. The only difference is the output spectrum level is reduced by 15 dB (=0.35dB/km × 43 km) due to fiber loss. The simulation results in Fig. 5 is repeated in Fig. 6 for
dBm and Lmax=63 km. Note that the spectrum at the fiber output is slightly distorted when compared with the spectrum at the fiber input. This distortion comes from the FWM effect.![]() | Figure 5. Optical power spectra corresponding to unamplified 32×224 Gbps O-band WDM system operating with 16-QAM signal and Ps=0 dBm. (a) At the fiber input. (b) After 43 km transmission |
and 8 dBm, respectively. The fiber length is set to Lmax which equals
km, respectively. Other parameters used in the simulation are
dBm and N = 32. Note that the effect of FWM on the output spectrum is more pronounced when compared with Fig. 5 and 6, especially, when
dBm.![]() | Figure 6. Optical power spectra corresponding to unamplified 32×224 Gbps O-band WDM system operating with 16-QAM signal and Ps=8 dBm. (a) At the fiber input. (b) After 63 km transmission |
![]() | Figure 7. Optical power spectra corresponding to unamplified 32×224 Gbps C-band WDM system operating with 16-QAM signal and Ps=0 dBm. (a) At the fiber input. (b) After 65 km transmission |
![]() | Figure 8. Optical power spectra corresponding to unamplified 32×224 Gbps C-band WDM system operating with 16-QAM signal and Ps=8 dBm. (a) At the fiber input. (b) After 60 km transmission |
onnumber of multiplexed channels for O-band and C-band, respectively. The results are reported for unamplified link with
dBm (inserted at the receiver side). The O-band operation reveals the following results(i) When the number of multiplexed channels N ≤ 16, the maximum transmission distance is almost independent of N. Further, Lmax increases with signal laser power Ps. When Ps=0 dBm, Lmax ≈ 44 km when N= 1, 4, 8, and 16. Increasing Ps to 10 dBm yields Lmax ≈ 68 km.(ii) Increasing N to 32 decreases Lmax to 43 km and 50 km, when Ps=0 and 10 dBm, respectively. Note also that Lmax increases with Ps and reaches 63 km when Ps=8 dBm. Increasing Ps above 8 dBm reduces the value of Lmax. This behavior can be attributed to FWM effect associated with fiber nonlinear optics. Therefore, one can conclude that the optimum value of Ps=8 dBm when N=32 which gives the longest possible reach of 63 km.![]() | Figure 9. Dependence of maximum reach of unamplified 16-QAM WDM system on number of multiplexed channels and assuming Pc=0 dBm and 224 Gbps 16-QAM channel data. (a) O-band. (b) C-band |
![]() | Figure 10. Configuration of an optical link with boost erbium-doped optical amplifier used in the experiment of Ref. [23] |
and the optical carrier-to-signal power ratio (CSPR) were taken as independent parameters in the results presented in Ref. [23]. From Fig.10. The optical signal lunched at the fiber input can be expressed as![]() | (26a) |
![]() | (26b) |
to a certain value, simulate the optical modulator subsystem, and record the SSB signal power
.(ii) Calculate the required carrier laser power
and EDFA gain
.(iii) Set the values of other system parameters related to the transmitter, transmission link, EDFAs, and receiver as those reported in Ref. [23].For example, to achieve
= 9 dBm and
dB as considered in the reference, the signal laser power is set to 5 dBm in the simulation. The simulation yields
dBm, and therefor, the carrier laser power is set to 3.5 dBm to achieve
dB. The total power at the coupler output equals
which corresponds to
dBm. The gain G of the boost EDFA is set to 5.3 dB to get a 9 dB lunch power. Under these settings, the simulation yields BERs of
, and
for B2B, one span, and two-span transmission respectively. These are to be compared with
, and
experimental BERs, respectively, as reported in Fig. 9c in Ref. [23]. Note that, both simulation and experimental BERs are lower than
, which represents the BER threshold for 7% HD-FEC code. Note further that the simulation BERs,
, are in the same order of the experimental ones,
where
. Figures 11 (a-c) show the simulated optical spectra after 0, 80, and 160 km transmission distance, respectively. The simulated and experimental constellation diagrams after 80 and 160 km are given in parts d and e of this figure.![]() | Figure 11. Spectra of (carrier + SSB) waveforms and constellation diagrams related to amplified 224 Gbps carrier-assisted 16-QAM system operating at C-band (carrier at transmitter). (a) Spetrum after 0 km transmission. (b) Spectrum after 80 km transmission. (c) Spectrum after 160 km transmission. (d) Simulated and experimental constellation diagrams after 80 km transmission. (e) Simulated and experimental constellation diagrams after 160 km transmission |
![]() | Figure 11. (Continued) |
![]() | Figure 12. Variation of BER with lunch power after 160 km transmission with of 14 dB |
and
, which are related to 20% and 7% HD-FEC codes, respectively. Chromatic-dispersion compensation (CDC) technique was used to compensate fiber dispersion. The experiment was repeated with digital back propagation (DBP) technique to compensate both fiber dispersion and fiber nonlinearity.To simulate the experimental system reported in [28], an assisted optical carrier is inserted in each of the WDM channel transmitters. Thus, each transmitter contains both signal and carrier lasers. This approach has two main effects. (i) The total power launched into the fiber will be increased leading to high fiber nonlinear optics effects. (ii) The spectrum of the signal at the output of the channel transmitter covers frequencies from
to
. For
Gbps and 16-QAM signaling
and
, the bandwidth of the transmitter signal
GHz. Therefore, channel spacing of 50 GHz with high-order 40 GHz demultiplexer bandpass filters are used to ensure negligible crosstalk in accord with the experimental results. For comparison purposes, the above experimental work is simulated here using Optisystem software with lunch power per channel
of 1 dBm and
of 10.2 dB. When
is set to 0 dBm, the simulation gives
dBm
. The carrier laser power
required to achieve a
of 10.2 dB is equals – 0.3 dB
The lunch power per channel
where G is the gain of the OA inserted after the multiplexer. Note that,
dBm. Therefore,
dB is used to yield
dBm.Figure 13 shows simulation results related to the system under observation when the transmission link consists of 4 spans (320 km). Parts a and b display the optical spectra at the input and output of the transmission link. Note, the output spectrum contains many intermodulation distortion components due to the effect of fiber nonlinearity. Parts c and d compare the power spectra at the transmitter output and receiver input of channel 1. The two spectra contain almost the same frequency content, which reflects the effectiveness of the receiver DSP unit in compensating chromatic dispersion and nonlinear fiber optics. This is clear further by comparing the constellation diagrams at the receiver before and after the DSP unit as shown in parts e and f of this figure, respectively.![]() | Figure 13. Optical power spectra and constellation diagrams corresponding to unamplified (8×100 Gbps) C-band WDM system operating with 16-QAM signal and Ps=0 dBm. (a) Spectrum at the fiber input. (b) Spectrum after 320 km transmission. (c) Spectrum at the transmitter output of channel 1. (d) Spectrum at the receiver input of channel 1. (e) Receiver constellation diagram at the DSP input. (f) Receiver constellation diagram at the DSP output |
is used. In fact, the simulation predicts successful transmission over 5 spans (400 km) as shown in Fig. 15 when
dBm and CSPR = 10.2 dB. Figures 15 also contains results corresponding to CSPR of 8.2 and 12.2 dB and included here to address the effect of CSPR or the channels BERs. Investigating the results in Fig. 4.13 reveals that at constant lunch power per channel
, using CSPR of 10.2 dB offers BERs less than the BER threshold for all the eight channels. Increasing CSPR on 12.2 dB or reducing CSPR to 8.2 dB increases the BERs of the channels and makes some of them above the BER threshold. This result can be explained as follows.
. Therefore,
and hence, increasing CSPR leads to increasing
The BER characteristics depends on the effective SNR, which can be stated as![]() | (27) |
. In this equation,
is proportionality constant,
represents the signal-independent noise power, and
represents the signal × signal beat interference. Taking the derivative of
with respect
and set it to zero yields
Note that, the optimum value of CSPR depends on channel lunch power
and system parameters (B1 and B2). If one considers a 10.2 dB is the optimum value of CSPR at
dB, then
. Thus, the actual
generated by the optical modulator
should by amplified by
before lunching it into the fiber. ![]() | Figure 14. Comparison between measured BERs [28] and simulated ones for all the 8 channels after 320 km transmission assuming Pch = 1 dBm and CSPR = 10.2 dB |
![]() | Figure 15. Simulated BERs of the 8 channels after 400 km transmission assuming Pch = 1 dBm |
![]() | Figure 16. Spectra and constellation diagrams related to an unamplified 224 Gbps 16-QAM system operating at 1550 nm wavelength with L=62 km, Ps=0 dBm and Pc=0 dBm (carrier at transmitter). (a) Spectrum of the QAM pulse generator output (-phase component). (b) Spectrum of the QAM modulator input. (c) Spectrum of the QAM modulator output. (d) Spectrum of the optical modulator output. (e) Spectrum of the optical SSB signal. (f) Spectrum of signal SSB + assisted carrier. (g) Spectrum of the optical signal at the fiber output. (h) Spectrum of the amplified photocurrent. (i) Spectrum of the QAM demodulator output. (j) Spectrum of the filtered QAM demodulator output. (k) Receiver constellation diagram at the DSP input. (L) Receiver constellation diagram at the DSP output |
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