COMPONENTS 193
Consider a wavelength for which the cavity length i.e., the distance between the two mirrors is an integral multiple of half the wavelength. That is, the round trip through
the cavity is an integral multiple of the wavelength. For such a wavelength, all of the light waves transmitted through the right facet are in phase; therefore, they reinforce each
other. Such a wavelength is called a resonant wavelength of the cavity.
Since there are many resonant wavelengths, the resulting output consists of many wavelengths spread over a few nm, with a gap between two adjacent wavelengths of
100 GHz to 200 GHz. However, it is desirable that only a single wavelength comes out from the laser. This can be done by using a filtering mechanism that selects the desired
wavelength and provides loss to the other wavelengths. Specifically, another cavity can be used after the primary cavity where gain occurs. Using reflective facets in the second
cavity, the laser can oscillate only at those wavelength resonant for both cavities.
If we are to make the length of the cavity very small, then only one resonant wavelength occurs. It turns out that such a cavity can be done on a semiconductor substrate. In this
case the cavity is vertical with one mirror on the top surface and the other in the bottom surface. This type of laser is called a vertical cavity surface emitting laser VCEL. Many
VCELs can be fabricated in a two-dimensional array.
Tunable lasers Tunable lasers are important to optical networks, as will be seen in the two subsequent
chapters. Also, it is more convenient to manufacture and stock tunable lasers, than make different lasers for specific wavelengths. Several different types of tunable lasers exist,
varying from slow tunability to fast tunability.
Modulation Modulation is the addition of information on a light stream. This can be realized using
the on-off keying OOK scheme. In this scheme, the light stream is turned on or off depending whether we want to modulate a 1 or a 0. OOK can be done using direct or
external modulation. In direct modulation, the light drive current into the semiconductor
laser is set above threshold for 1 and below it for a 0. As a result, the presence of high or low power is interpreted as a 1 or 0, respectively. Direct modulation is easy
and inexpensive to implement. However, the resulting pulses become chirped; that is, the carrier frequency of the transmitted pulse varies in time.
External modulation is achieved by placing an external modulator in front of a laser. The laser continuously transmits but the modulator either lets the light through or stops
it accordingly if it is a 1 or a 0. Thus, the presence of light is interpreted as a 1 and no light is interpreted as a 0. An external modulator minimizes chirp.
Dense WDM DWDM In the literature, the term dense WDM DWDM is often used. This term does not imply a
different technology to that used for WDM. In fact, the two terms are used interchangeably. Strictly speaking, DWDM refers to the wavelength spacing proposed in the ITU-T G.692
standard. Originally, the wavelengths were separated by wide bands which were several tens or hundreds of nanometers. These band became very narrow as technology improved.
194 OPTICAL FIBERS AND COMPONENTS
Table 8.2 ITU-T DWDM grid.
Channel code
λ
nm Channel
code
λ
nm Channel
code
λ
nm Channel
code
λ
nm
18 1563.05
30 1553.33
42 1543.73
54 1534.25
19 1562.23
31 1552.53
43 1542.94
55 1533.47
20 1561.42
32 1551.72
44 1542.14
56 1532.68
21 1560.61
33 1590.12
45 1541.35
57 1531.90
22 1559.80
34 1550.12
46 1540.56
58 1531.12
23 1558.98
35 1549.32
47 1539.77
59 1530.33
24 1558.17
36 1548.52
48 1538.98
60 1529.55
25 1557.36
37 1547.72
49 1538.19
61 1528.77
26 1556.56
38 1546.92
50 1537.40
62 1527.99
27 1555.75
39 1546.12
51 1536.61
– –
28 1554.94
40 1545.32
52 1535.82
– –
29 1554.13
41 1544.53
53 1535.04
– –
ITU-T proposed a set of closely spaced wavelengths in the 1550 nm window. The reason that the 1550 nm window was chosen is due to the fact that it has the smallest amount
of attenuation and it also lies in the band where the Erbium-doped fiber amplifier see Section 8.3.3 operates. The ITU-T proposed guard is 0.8 nm or 100 GHz and the grid is
centered in 1552.52 nm or 193.1 THz. The ITU-T grid is given in Table 8.2. The ITU-T grid is not always followed, since there are many proprietary solutions.
Note that this book uses the acronym WDM.
8.3.2 Photo-detectors and Optical Receivers
Let us consider the receiving side of the WDM link see Figure 8.16. The WDM optical signal is demultiplexed into the W different wavelengths, and each wavelength is directed
to a receiver Rx. The demultiplexer is a 1-to-N splitter see Section 8.3.3. Each receiver consists of a photodetector, an amplifier, and a signal-processing circuit. The photode-
tector senses an optical signal and produces an electrical signal that contains the same information as in the optical signal. The electrical signal is subsequently amplified so that
it can be processed electronically by the signal-processing circuit.
8.3.3 Optical Amplifiers
The optical signal looses its power as it propagates through an optical fiber, and after some distance it becomes too weak to be detected Section 8.2.2. Optical amplification
is used to restore the strength of the signal. Optical amplification can be used as power amplifiers, in-line amplifiers, and preamplifiers, in a WDM link Figure 8.16. The optical
signal can be boosted after it leaves the multiplexer, and before it enters the receiver. In- line amplifiers are used for very long transmission WDM links, and they typically boost the
power of the signal to compensate for what was lost prior to entering the optical amplifier.
Prior to optical amplifiers, the optical signal was regenerated by first converting it into an electrical signal, then apply 1R or 2R or 3R regeneration, and then converting the
COMPONENTS 195
regenerated signal back into the optical domain. In 1R, the electrical signal is simply re-amplified, in 2R, the signal is re-amplified and re-shaped, and in 3R, the signal is re-
amplified, re-shaped, and re-timed. In order to re-amplify or re-shape an electrical signal, we do not need to have knowledge of its bit-rate and frame format. However, for re-timing
knowledge of both the bit-rate and frame format is necessary.
Optical amplification, as in the 1R scheme, can be done without knowledge of the bit rate and the framing format, and it can be applied simultaneously to the combined signal
of all of the wavelengths in a WDM link. Currently, re-shaping and re-timing cannot be done in the optical domain. There are several different types of optical amplifiers, such
as the Erbium-doped fiber amplifier EDFA, the semiconductor optical amplifier SOA and the Raman amplifier. Below, we describe the Erbium-doped fiber amplifier, a key
technology that enabled the deployment of WDM systems. The SOA is mostly used in optical cross-connects OXCs
and is described in Section 8.3.5. The Erbium-doped fiber amplifier EDFA
The EDFA consists of a length of silica fiber whose core is doped with Erbium, a rare earth element. As shown in Figure 8.18, a laser is emitted into the fiber and is combined
through a coupler see Section 8.3.4 with the signal that needs to be amplified. This laser operates at 980 nm or 1480 nm, and the signal to be amplified is in the 1550 nm window.
The signal from the laser pumps the doped fiber and induces a stimulated emission of the electrons in the fiber. That is, electrons are induced to transmit from a higher energy
level to a lower energy level, which causes the emission of photons, and which in turn amplifies the incoming signal. An isolator is used at the input andor output to prevent
reflections into the amplifier.
In practice, EDFAs are more complex than the one shown in Figure 8.18; the two-stage EDFA shown in Figure 8.19 is much more common. In the first stage, a co-directional
Laser 850 nm
Signal to be amplified
1550 nm Coupler
Erbium- doped fiber
Isolator Isolator
Figure 8.18 The Erbium-doped fiber amplifier.
Signal to be amplified
1550 nm Isolator Isolator
Coupler Coupler
Erbium- doped fiber
Laser 850
Laser 850
Figure 8.19 A two-stage EDFA.
196 OPTICAL FIBERS AND COMPONENTS
laser pumps into the coupler in the same direction as the signal to be amplified, and in the second stage, a counter-directional laser pumps into the coupler in the opposite
direction of the signal to be amplified. Counter-directional pumping gives higher gain, but co-directional pumping gives better noise performance.
8.3.4 The 2 × 2 Coupler
The 2 × 2 coupler is a basic device in optical networks, and it can be constructed in variety of different ways. A common construction is the fused-fiber coupler. This is fabricated
by twisting together, melting, and pulling two single-mode fibers so that they get fused together over a uniform section of length. Each input and output fiber has a long tapered
section see Figure 8.20.
Let us assume that an input light is applied to input 1 of fiber 1. As the input light propagates through the fiber 1 tapered region into the coupling region, an increasing
portion of the input electric field propagates outside of the fiber 1 core and is coupled into fiber 2. A negligible amount of the incoming optical power is reflected back into
the fibers. In view of this, this type of coupler is known as a directional coupler. The optical power coupled from one fiber to the other can be varied by varying the length of
the coupling region, the size of the reduced radius of the core in the coupling region, and the difference in the radii of the two fibers in the coupling region. There is always some
power loss when the light goes through the coupler.
A more versatile 2 × 2 coupler is the waveguide coupler see Figure 8.21. A waveguide
is a medium that confines and guides a propagating electromagnetic wave. A
Coupling region
Tapered region
Tapered region
Input 1 Output 1
Output 2 Fiber 1
Fiber 2 Input 2
Figure 8.20 A fused-fiber 2 × 2 coupler.
Coupling region
Input 1 Output 1
Output 2 Input 2
Figure 8.21 A 2 × 2 waveguide coupler.