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Chapter 2: Literature Review
enabling the fibre feeder network to support the required large number of BSs to
service a certain geographical area.
The introduction of OSSB+C modulation as well as tandem single sideband
modulation enables increased spectral efficiency by reducing the required spectralband for an optical mm-wave channel, in addition to mitigating the effect of fibre
chromatic dispersion due to ODSB+C modulation format [59-61,112-122]. The
tandem single sideband modulation effectively doubles the capacity of the mm-wave
fibre-radio systems while compared to the conventional ODSB+C based systems
[121-122]. However, the use of WDM in fibre feeder networks can resolve the
challenge by enabling transport of multiple optically modulated mm-wave signals,
feeding multiple antenna BSs through one fibre [15-16, 23, 36-39] . The following
section reviews the literatures towards the implementation of WDM fibre feeder
network in mm-wave fibre-radio systems.
2.3.1 Wavelength Division Multiplexed MM-Wave Fibre-Radio
WDM is an elegant and effective way to increase the capacity of the fibre optic
feeder networks in mm-wave fibre radio systems. In the WDM incorporated feeder
networks, optical mm-wave channels, each carried by a separate wavelength, are
transmitted to/from the BSs via the CO through a single fibre that provides quantum
increase in network capacity without the need for laying new fibre [15-16, 23, 36-39,
44, 89, 92-93, 123-129]. It also simplifies the network upgrades and the deployment
of additional BSs, while support multiple interactive services for future broadband
wireless access communications [15, 36-37, 125-126].
Fig. 2.12 shows the general concept of a typical mm-wave fibre-radio system
incorporating WDM. In the downlink direction, optical mm-wave channels, spaced at
an effective WDM separation, are generated in the CO by using WDM optical
sources, and are passed through a suitable multiplexer that aggregates them to a
composite signal. The multiplexed signals are then transported over optical fibre to
the remote nodes (RN), where the individual optical mm-wave signals are
demultiplexed and directed to antenna BSs for mm-wave wireless distribution. In the
uplink direction, mm-wave signals generated at the customer sites are converted
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Chapter 2: Literature Review
CO
Remote Node
(RN)
BS1
BS2
BSN
BS1
BS2
BSN
CO
Remote Node
(RN)
BS1
BS2
BSN
BS1
BS2
BSN
Fig.2.12: Schematic diagram of typical mm-wave fibre-radio feeder network incorporating WDM
from electrical-to-optical form at BSs and sent to the RN, where the optically
modulated signals are multiplexed before directed to the CO through fibre for further
processing. Such fibre-radio feeder network enables a large number of BSs remotely
share the switching and signal processing hardware located at the CO, in addition to
simplifying the complexity of BSs by enabling passive multiplexing and
demultiplexing functionality at the RNs. Since each of the optical mm-wave channels
are effectively separated from others, they can be independent in protocol, speed, and
direction of communication. As mentioned in Chapter 1, it is envisaged that future
wireless bandwidth will be met by mm-wave WDM fibre-radio systems, where each
of the remote antenna BS will be allocated a WDM optical carrier to transport the
optically modulated mm-wave signals to/from the CO through the fibre optic feeder
network, irrespective of direction of communication. However, using the same
wavelength for both downlink and uplink communication is not any requirement,
since channel offset scheme as well as interleaved downlink and uplink channels can
also be used.
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Chapter 2: Literature Review
With the maturity of WDM components and system technologies, the effective
WDM channel separations in the conventional optical access and metro domain are
gradually replaced with dense-wavelength-division-multiplexing (DWDM)
separations of 100 GHz, 50 GHz, and 25 GHz. The introduction of DWDM fibre
feeder networks in mm-wave fibre-radio systems may surprisingly increase the
capacity of the systems by supporting huge number of BSs required for future
multiple interactive broadband wireless services. Also, it is important that mm-wave
fibre-radio systems can coexist with other conventional DWDM access and metro
technologies, as it is expected that mm-wave fibre-radio systems will be realised by
utilising the unused capacity of the existing optical infrastructure in the access or
metro domain, instead of deploying separate fibre-radio backbone. However, the
inherent wideband characteristics of mm-wave signals (25-100 GHz) impose spectral
restrictions in realising fibre feeder network with a channel separation ≤ 100 GHz.
Fig. 2.13 shows the optical spectra of OSSB+C modulated N optical mm-wave
channels with a WDM channel separation and a mm-wave carrier frequency of
∆fWDM and ∆fmm-wave respectively, where ∆fmm-wave < ∆fWDM . In order to realise
DWDM fibre feeder networks for mm-wave fibre-radio systems, in most of the
cases, it is necessary to reduce ∆fWDM < ∆fmm-wave, which has been an active area for
∆fmm-wave
∆fWDM
S1
C1
S2
C2
SN
CN
∆fmm-wave
∆fWDM
S1
C1
S2
C2
SN
CN
Fig. 2.13: Optical spectra of the N optical mm-wave channels in a WDM feeder network for mmwave fibre-radio systems.
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