Optical Networks: A Practical Perspective - Part 11 ppsx

Broadening of Chirped Gaussian Pulses Figure 2.9 shows the pulse-broadening effect of chromatic dispersion graphically.. The dispersion length for a 2.5 Gb/s system operating over stand

I

Figure 2.8 A (negatively) chirped Gaussian pulse Here, and in all such figures, we show the shape of the pulse as a function of time

unchirped pulses to acquire a chirp It then becomes important to study the effect of chromatic dispersion on such pulses The third reason is that the best transmission performance is achieved today by the use of Gaussian pulses that are deliberately chirped (We will discuss these systems in Section 2.5.1 and in Chapter 5.)

Pulses with a Gaussian envelope are used in high-performance systems employing

RZ modulation (see Section 4.1) For most other systems, the pulses used tend to be rectangular rather than Gaussian However, the results we derive will be qualitatively valid for most pulse envelopes In Appendix E, we describe mathematically how chirped Gaussian pulses propagate in optical fiber The key result that we will use in subsequent discussions here is that after a pulse with initial width To has propagated

a distance z, its width Tz is given by

_ _ rz ] + Ki32z + I32z ] 2

(2.13)

Here K is called the chirp factor of the pulse and is proportional to the rate of change

of the pulse frequency with time (A related parameter, which depends on both the chirp and the pulse rise-time, is called the source frequency chirp factor, c~, in the Telcordia SONET standard GR.253.)

Broadening of Chirped Gaussian Pulses

Figure 2.9 shows the pulse-broadening effect of chromatic dispersion graphically In these figures, the center or carrier frequency of the pulse, coo, has deliberately been shown greatly diminished for the purposes of illustration We assume/32 is negative; this is true for standard single-mode fiber in the 1.55 lzm band Figure 2.9(a) shows

an unchirped (K = 0) Gaussian pulse, and Figure 2.9(b) shows the same pulse after

After distance 2 L D

-4

After distance 0.4 L D

Figure 2.9 Illustration of the pulse-broadening effect of chromatic dispersion on

unchirped and chirped Gaussian pulses (for/~2 < 0) (a) An unchirped Gaussian pulse at

z = 0 (b) The pulse in (a) at z = 2Lb (c) A chirped Gaussian pulse with x = - 3 at z = 0 (d) The pulse in (c) at z = 0.4Lb For systems operating over standard single-mode fiber

at 1.55/,m, LD ,~ 1800 km at 2.5 Gb/s, whereas LD ,~ 115 km at 10 Gb/s

it has propagated a distance 2T2/1,821 along the fiber Figure 2.9(c) shows a chirped Gaussian pulse with K = - 3 , and Figure 2.9(d) shows the same pulse after it has propagated a distance of only 0.4T2/j,821 along the fiber The amount of broadening can be seen to be about the same as that of the unchirped Gaussian pulse, but the distance traveled is only a fifth This shows that the presence of chirp significantly exacerbates the pulse broadening due to chromatic dispersion (when the product Kfl2

is positive)

The quantity T2/I/~21 is called the dispersion length and is denoted by LD It serves as a convenient normalizing measure for the distance z in discussing the effects of chromatic dispersion For example, the effects of chromatic dispersion can

be neglected if z << LD since in that case, from (2.13), Tz/To ~ 1 It also has the interpretation that the width of an unchirped pulse at the 1/e-intensity point increases

by a factor of C~ after it has propagated a distance equal to the dispersion length

(a) (b)

Figure 2.10 Illustration of the pulse compression effect of chromatic dispersion when K/32 < 0 (a) A chirped Gaussian pulse with k: = - 3 at z = 0 (b) The pulse in (a) at

z = 0.4LD

The dispersion length for a 2.5 Gb/s system operating over standard single-mode fiber at 1.55 # m is approximately 1800 km, assuming To = 0.2 ns, which is half the bit interval If the bit rate of the system is increased to 10 Gb/s with To = 0.05 ns, again half the bit interval, the dispersion length decreases to approximately 115 km This indicates that the limitations on systems due to chromatic dispersion are much more severe at 10 Gb/s than at 2.5 Gb/s We will discuss the system limitations of chromatic dispersion in Section 5.7.2 (The chromatic dispersion limit at 2.5 Gb/s is considerably shorter, about 600 km, than the dispersion length of 1800 km because

N R Z pulses are used.)

For I( = 0 and z = 2LD, (2.13) yields Tz/To = ~/5 ~ 2.24 For a: = - 3 and

z = 0.4LD, (2.13) yields Tz/To = ~/5 ~ 2.24 Thus both pulses broaden to the same

extent, and these values are in agreement with Figure 2.9

An interesting phenomenon occurs when the product Kfl2 is negative The pulse initially undergoes compression up to a certain distance and then undergoes broaden- ing This is illustrated in Figure 2.10 The pulse in Figure 2.10(a) is the same chirped Gaussian pulse shown in Figure 2.9(c) and has the chirp parameter K = - 3 But the sign of/~2 is now positive (which is the case, for example, in the lower portion of the

1.3 lzm band), and the pulse, after it has propagated a distance z = 0.4Ln, is shown

in Figure 2.10(b) The pulse has now undergone compression rather than broad-

ening This can also be seen from (2.13) since we now get Tz/To = 1/~/5 ~ 0.45

However, as z increases further, the pulse will start to broaden quite rapidly This can be seen from Figure 2.11, where we plot the pulse width evolution as a function

of distance for different chirp parameters (Also see Problem 2.11.) We will discuss this phenomenon further in Sections 2.4.5 and 2.4.6

2.5

K = - - I

~"~ 1.5

0.5

z / L D

Figure 2.11 Evolution of pulse width as a function of distance ( z / L D ) for chirped and unchirped pulses in the presence of chromatic dispersion We assume f12 < 0, which is the case for 1.55 #m systems operating over standard single-mode fiber Note that for positive chirp the pulse width initially decreases but subsequently broadens more rapidly For systems operating over standard single-mode fiber at 1.55/~m, L D ~ 1800 km at 2.5 Gb/s, whereas L D ~'~ 115 km at 10 Gb/s

An intuitive explanation of pulse compression and broadening due to chromatic dispersion is as follows For a negatively chirped pulse, the instantaneous frequency decreases with increasing time, as illustrated in Figures 2.9(c) and 2.10(a) When /32 > 0, higher-frequency (components of) pulses travel faster than lower-frequency (components of) pulses, and vice versa Thus, when f12 > 0, the tail of the pulse, which has higher-frequency components, travels faster than the head of the pulse, which has lower-frequency components, resulting in pulse compression This is the situation illustrated in Figure 2.10 When/32 < 0, the situation is reversed: the tail

of the pulse travels slower than the head of the pulse, and the pulse broadens This

is the situation illustrated in Figure 2.9(c) and (d)

The pulse compression phenomenon can be used to increase the transmission distance before chromatic dispersion becomes significant, if the sign of Kfl2 can

be made negative Since the output of directly modulated semiconductor lasers is negatively chirped, the fiber must have a positive/32 for pulse compression to occur While standard single-mode fiber cannot be used because it has negative/32 in the

been designed specifically to take advantage of this pulse compression effect in the design of metropolitan systems

acquires chirp when it has propagated some distance along the fiber Furthermore, the acquired chirp is negative since the frequency of the pulse decreases with increasing time, t The derivation of an expression for the acquired chirp is left as an exercise (Problem 2.9)

2.3.2 Controlling the Dispersion Profile

Group velocity dispersion is commonly expressed in terms of the chromatic disper- sion parameter D that is related to/32 as D = - (27rc/)~2)f12 The chromatic dispersion

parameter is measured in units of ps/nm-km since it expresses the temporal spread (ps) per unit propagation distance (km), per unit pulse spectral width (nm) D can

be written as D - DM + Dw, where DM is the material dispersion and Dw is the

waveguide dispersion, both of which we have discussed earlier Figure 2.12 shows

DM, Dw, and D for standard single-mode fiber DM increases monotonically with

~ and equals 0 for ~ = 1.276/zm On the other hand, Dw decreases monotonically

with )~ and is always negative The total chromatic dispersion D is zero around

~ = 1.31 ~m; thus the waveguide dispersion shifts the zero-dispersion wavelength

30

10

r ~

&

~ 0

0

~ -10

r ~

,, ~

-20

1.1

Material

_ll~ _~J ~.dispersion

l~2 > u dispersion dispersion tJ2 < u

, , , | i , | | , l | , , , i i i , , , , I

Wavelength, ~ (~tm)

Figure 2.12 Material, waveguide, and total dispersion in standard single-mode optical fiber Recall that chromatic dispersion is measured in units of ps/nm-km since it expresses the temporal spread (ps) per unit propagation distance (km), per unit pulse spectral width (nm) (After [Agr97].)

by a few tens of nanometers Around the zero-dispersion wavelength, D may be approximated by a straight line whose slope is called the chromatic dispersion slope

of the fiber

For standard single-mode fiber, the chromatic dispersion effects are small in the 1.3 # m band, and systems operating in this wavelength range are loss limited On the other hand, most optical communication systems operate in the 1.55 # m band today because of the low loss in this region and the well-developed erbium-doped fiber amplifier technology But as we have already seen, optical communication systems in this band are chromatic dispersion limited This limitation can be reduced

if somehow the zero-dispersion wavelength were shifted to the 1.55 # m band

We do not have much control over the material dispersion DM though it can

be varied slightly by doping the core and cladding regions of the fiber How- ever, we can vary the waveguide dispersion Dw considerably so as to shift the zero-dispersion wavelength into the 1.55 # m band Fibers with this property are called dispersion-shifted fibers (DSF) Such fibers have a chromatic dispersion of at most 3.3 ps/nm-km in the 1.55 # m wavelength range and typically zero dispersion

Recall that when/32 > 0, the chromatic dispersion is said to be normal, and when /32 < 0, the chromatic dispersion is said to be anomalous Pulses in silica fiber expe- rience normal chromatic dispersion below the zero-dispersion wavelength, which is around 1.3 # m for standard single-mode fiber Pulses experience anomalous disper- sion in the entire 1.55 # m band in standard single-mode fiber For dispersion-shifted fiber, the dispersion zero lies in the 1.55 # m band As a result, pulses in one part of

part of the band experience anomalous chromatic dispersion

The waveguide dispersion can be varied by varying the refractive index profile

of the fiber, that is, the variation of refractive index in the fiber core and cladding A typical refractive index profile of a dispersion-shifted fiber is shown in Figure 2.13(b) Comparing this with the refractive index profile of a step-index fiber shown in Fig- ure 2.13(a), we see that, in addition to a trapezoidal variation of the refractive index

in the fiber core, there is step variation of the refractive index in the cladding Such

a variation leads to a single-mode fiber with a dispersion zero in the 1.55 # m band

As we will see in Section 5.7.3, fibers with very large chromatic dispersions (but with the opposite sign) are used to compensate for the accumulated chromatic dispersion on a lengthy link The refractive index profile of such a fiber is shown

in Figure 2.13(c) The core radius of such a fiber is considerably smaller than that

of standard single-mode fiber but has a higher refractive index.This leads to a large negative chromatic dispersion This core is surrounded by a ring of lower refractive index, which is in turn surrounded by a ring of higher refractive index Such a

Di~ ,tance from core center

(a)

Distance from core center Distance from core center

Figure 2.13 Typical refractive index profile of (a) step-index fiber, (b) dispersion-shifted fiber, and (c) dispersion-compensating fiber (After [KK97, Chapter 4].)

variation leads to a negative chromatic dispersion slope, an important characteristic for chromatic dispersion compensation, as we will see in Section 5.7.3

2.4 Nonlinear Effects

Our description of optical communication systems under the linearity assumption

we made in Section 2.1.2 is adequate to understand the behavior of these systems when they are operated at moderate power (a few milliwatts) and at bit rates up to about 2.5 Gb/s However, at higher bit rates such as 10 Gb/s and above and/or at higher transmitted powers, it is important to consider the effect of nonlinearities In the case of WDM systems, nonlinear effects can become important even at moderate powers and bit rates

There are two categories of nonlinear effects The first arises due to the interaction

of light waves with phonons (molecular vibrations) in the silica medium one of several types of scattering effects, of which we have already met one, namely, Rayleigh scattering (Section 2.2) The two main effects in this category are stimulated Brillouin scattering (SBS) and stimulated Raman scattering (SRS)

The second set of nonlinear effects arises due to the dependence of the refractive index on the intensity of the applied electric field, which in turn is proportional to the square of the field amplitude The most important nonlinear effects in this category are self-phase modulation (SPM) and four-wave mixing (FWM)

In scattering effects, energy gets transferred from one light wave to another wave at a longer wavelength (or lower energy) The lost energy is absorbed by the molecular vibrations, or phonons, in the medium (The type of phonon involved is different for SBS and SRS.) This second wave is called the Stokes wave The first wave can be thought of as being a "pump" wave that causes amplification of the

2.4.1

Stokes wave As the pump propagates in the fiber, it loses power and the Stokes wave gains power In the case of SBS, the pump wave is the signal wave, and the Stokes wave is the unwanted wave that is generated due to the scattering process In the case of SRS, the pump wave is a high-power wave, and the Stokes wave is the signal wave that gets amplified at the expense of the pump wave

In general, scattering effects are characterized by a gain coefficient g, measured

in meters per watt, and spectral width A f over which the gain is present The gain coefficient is a measure of the strength of the nonlinear effect

In the case of self-phase modulation, the transmitted pulses undergo chirping This induced chirp factor becomes significant at high power levels We have al- ready seen in Section 2.3 that the pulse-broadening effects of chromatic dispersion can be enhanced in the presence of chirp Thus the SPM-induced chirp can signif- icantly increase the pulse spreading due to chromatic dispersion in these systems For high-bit-rate systems, the SPM-induced chirp can significantly increase the pulse spreading due to chromatic dispersion even at moderate power levels The precise effects of SPM are critically dependent not only on the sign of the GVD parameter /32 but also on the length of the system

In a WDM system with multiple channels, the induced chirp in one channel depends on the variation of the refractive index with the intensity on the other channels This effect is called cross-phase modulation (CPM) When we discuss the induced chirp in a channel due to the variation of the refractive index with the intensity on the same channel, we call the effect SPM

In the case of WDM systems, another important nonlinear effect is that of four-wave mixing If the WDM system consists of frequencies fl, , fn, four-wave mixing gives rise to new signals at frequencies such as 2fi - f j and fi + f j fk

These signals appear as crosstalk to the existing signals in the system These crosstalk effects are particularly severe when the channel spacing is tight Reduced chromatic dispersion enhances the crosstalk induced by four-wave mixing Thus systems using dispersion-shifted fibers are much more affected by four-wave mixing effects than systems using standard single-mode fiber

We will devote the rest of this section to a detailed understanding of the various types of fiber nonlinearities

Effective Length and Area

The nonlinear interaction depends on the transmission length and the cross-sectional area of the fiber The longer the link length, the more the interaction and the worse the effect of the nonlinearity However, as the signal propagates along the link, its power decreases because of fiber attenuation Thus, most of the nonlinear effects occur early in the fiber span and diminish as the signal propagates

Po

Power

Po

Power

Link length

Figure 2.14 Effective transmission length calculation (a) A typical distribution of the

power along the length L of a link The peak power is Po (b) A hypothetical uniform distribution of the power along a link up to the effective length Le This length Le is

chosen such that the area under the curve in (a) is equal to the area of the rectangle in

(b)

Modeling this effect can be quite complicated, but in practice, a simple model that

assumes that the power is constant over a certain effective length L e has proved to be

quite sufficient in understanding the effect of nonlinearities Suppose Po denotes the power transmitted into the fiber and P (z) = Poe -~z denotes the power at distance z

along the link, with a being the fiber attenuation Let L denote the actual link length

Then the effective length (see Figure 2.14) is defined as the length Le such that

Z=0 This yields

1 - e - a L

Ol

Typically, a = 0.22 dB/km at 1.55/zm wavelength, and for long links where L >> 1/a,

we have L e ~ 20 km

In addition to the link length, the effect of a nonlinearity also grows with the intensity in the fiber For a given power, the intensity is inversely proportional to the area of the core Since the power is not uniformly distributed within the cross

section of the fiber, it is convenient to use an effective cross-sectional a r e a A e (see Figure 2.15), related to the actual area A and the cross-sectional distribution of the fundamental mode F(r, 0), as

Intensity Intensity

Figure 2.15 Effective cross-sectional area (a) A typical distribution of the signal inten- sity along the radius of optical fiber (b) A hypothetical intensity distribution, equivalent

to that in (a) for many purposes, showing an intensity distribution that is nonzero only for an a r e a Ae around the center of the fiber

where r and 0 denote the polar coordinates The effective area, as defined above, has the significance that the dependence of most nonlinear effects can be expressed

in terms of the effective area for the fundamental mode propagating in the given type of fiber For example, the effective intensity of the pulse can be taken to be

Ie = P / A e , where P is the pulse power, in order to calculate the impact of certain nonlinear effects such as SPM, as we will see below The effective area of SMF is around 85/zm 2 and that of DSF around 5 0 / z m 2 The dispersion compensating fibers that we will study in Section 5.7.3 have even smaller effective areas and hence exhibit higher nonlinearities

In the case of SBS, the phonons involved in the scattering interaction are acoustic phonons, and the interaction occurs over a very narrow line width of AfB = 20 MHz

at 1 5 5 / z m Also the Stokes and pump waves propagate in opposite directions Thus SBS does not cause any interaction between different wavelengths, as long as the wavelength spacing is much greater than 20 MHz, which is typically the case SBS can, however, create significant distortion within a single channel SBS produces gain

in the direction opposite to the direction of propagation of the signal, in other words, back toward the source Thus it depletes the transmitted signal as well as generates a potentially strong signal back toward the transmitter, which must be shielded by an isolator The SBS gain coefficient gB is approximately 4 x 10 -11 m/W, independent

of the wavelength