SOLUTION MANUAL FOR OPTICAL FIBER COMMUNICATIONS 4TH EDITION BY GERD KEISER€¦ · ·...
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Transcript of SOLUTION MANUAL FOR OPTICAL FIBER COMMUNICATIONS 4TH EDITION BY GERD KEISER€¦ · ·...
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SOLUTION MANUAL FOR OPTICAL FIBER COMMUNICATIONS 4TH
EDITION BY GERD KEISER
Gerd Keiser, Optical Fiber Communications, McGraw-Hill, 4th
ed., 2011 Problem Solutions for Chapter 2
2.1
E 1 00co s 2 1 08 t 3 0 ex 2 0co s 21 08t 5 0 ey
4 0co s 21 08 t 2 10 ez
2.2 The general form is:
y = (amplitude) cos(t - kz) = A cos [2(t - z/)]. Therefore
(a) amplitude = 8 m
(b) wavelength: 1/ = 0.8 m-1
so that = 1.25 m (c) = 2(2) = 4
(d) At time t = 0 and position z = 4 m we have
y = 8 cos [2(-0.8 m-1
)(4 m)]
= 8 cos [2(-3.2)] = 2.472
2.3 x1 = a1 cos (t - 1) and x2 = a2 cos (t - 2)
Adding x1 and x2 yields
x1 + x2 = a1 [cos t cos 1 + sin t sin 1]
+ a2 [cos t cos 2 + sin t sin 2]
= [a1 cos 1 + a2 cos 2] cos t + [a1 sin 1 + a2 sin
2] sin t Since the a's and the 's are constants, we can set
a1 cos 1 + a2 cos 2 = A cos (1)
a1 sin 1 + a2 sin 2 = A sin (2)
provided that constant values of A and exist which satisfy these
equations. To verify this, first we square both sides and add:
1
A2
(sin2
+ cos2
) = a
2 2
1 cos
2
1 1 sin
+
2 2
cos
2
2 + 2a1a2 (sin 1 sin 2 a2 sin 2
or
A2
= a 2 a 2 + 2a a cos ( - )
1 2 1 2 1 2
Dividing (2) by (1) gives
tan =
a 1
sin a 2 sin
1 2
a cos a cos
1 2
1 2
Thus we can write
x = x1 + x2 = A cos cos t + A sin
2.4 First expand Eq. (2.3) as
E y = cos (t - kz) cos - sin (t - kz) sin
E
0 y
Subtract from this the expression
E x cos = cos (t - kz) cos
E
0 x
to yield
Ey - E x
cos = - sin (t - kz) sin
E0 y
E0x
+ cos 1 cos 2)
sin t = A cos(t - )
(2.4-1)
(2.4-2)
Using the relation cos2
+ sin2
= 1, we use Eq. (2.2) to write
sin2
(t - kz) = [1 - cos2
(t - kz)] =
E
1 2 x
E
0x
(2.4-3)
Squaring both sides of Eq. (2.4-2) and substituting it into Eq. (2.4-3) yields
2
E y
E
0 y
E x
E 0x
2
cos
=
E 1 x
E
0x
2
sin2
Expanding the left-hand side and rearranging terms yields
2
2
E E E E
x
+ y
- 2 x y
E 0x E 0y E 0x E 0y
2.5 Plot of Eq. (2.7).
2.6 Linearly polarized wave.
2.7
Air: n = 1.0
33 33
Glass 90
cos = sin2
(a) Apply Snell's law
n1 cos 1 = n2 cos 2
where n1 = 1, 1 = 33, and 2 = 90 - 33 = 57
n2 = cos 33
= 1.540
cos 57
(b) The critical angle is found from
nglass
sin glass
= nair
sin air
with air = 90 and nair = 1.0
critical = arcsin 1
= arcsin 1
= 40.5n
g lass 1.540
3
4
2.8
Air r
Water
12 cm
Find c from Snell's law n1 sin 1 = n2 sin c = 1
When n2 = 1.33, then c = 48.75
Find r from tan c = r
, which yields r = 13.7 cm. 12 cm
2.9
45
Using Snell's law nglass sin c = nalcohol sin 90
where c = 45 we have n
glass = 1.45
= 2.05
sin 45
2.10 critical= arcsin
n
pure
= arcsin n
doped
1.450 1.460
= 83.3
2.11 Need to show that n1 cos 2 n 2 cos 1 0 . Use Snell’s Law and the relationship
tan sin
cos
5
2 2
2.12 (a) Use either NA = n1 n2
or
NA n1 2= n1 2(n1 n2
n1
1/ 2
= 0.242
) = 0.243
(b) A = arcsin (NA/n) = arcsin
0.242
1.0
= 14
1 n 2 1 1.00 2.13 (a) From Eq. (2.21) the critical angle is c sin sin 41
n
1.50
1
(c) The number of angles (modes) gets larger as the wavelength decreases.
2 2 1/ 2 2 2
(12.14 NA = n1 n2 = n1 n1
= n1
2 1 / 2
2
Since << 1, 2
<< ;
2.15 (a) Solve Eq. (2.34a) for jH:
)2 1/ 2
NA
n1
2
jH = j
Er -
1 Hz
r
Substituting into Eq. (2.33b) we have
j Er + E
rz =
Solve for Er and let
Er 1 H j z
r
q2
= 2 -
2 to obtain Eq. (2.35a).
(b) Solve Eq. (2.34b) for jHr:
jHr = -j
E -
1 Hz
Substituting into Eq. (2.33a) we have
r
6
1 E j E +
z = - j E
r
Solve for E and let q2
= 2
(c) Solve Eq. (2.34a) for jEr:
1 H z
r
- 2 to obtain Eq. (2.35b).
1 1 H
z
jEr =
jrH
Substituting into Eq. (2.33b) we have r
1 E H
z
z
jrH +
= jH
r
r
Solve for H and let q2
= 2 -
2 to obtain Eq. (2.35d).
(d) Solve Eq. (2.34b) for jE
jE= - 1
H z
jH r
r
1 E H - jHr
z
z
r r
Solve for Hr to obtain Eq. (2.35c).
Substituting into Eq. (2.33a) we have
(e) Substitute Eqs. (2.35c) and (2.35d) into Eq. (2.34c)
j 1 Hz
Ez
Hz
Ez
- r
= jE
z
2
q
r
r r
r
r
Upon differentiating and multiplying by jq2
/ we obtain Eq. (2.36).
7
(f) Substitute Eqs. (2.35a) and (2.35b) into Eq. (2.33c)
j 1
Ez
Hz Ez
Hz
= -jHz - 2 r q r r r r
r
Upon differentiating and multiplying by jq2
/ we obtain Eq. (2.37).
2.16 For = 0, from Eqs. (2.42) and (2.43) we have
Ez = AJ0(ur)
e j(t z )
and Hz = BJ0(ur)
e j(t z )
We want to find the coefficients A and B. From Eq. (2.47) and
(2.51), respectively, we have
C =
J
K
(ua) (wa)
A and D =
J
K
(ua) (wa)
B
Substitute these into Eq. (2.50) to find B in terms of A:
A
j 1
a 2
u
1
w 2
= B
J' (ua) K' (wa)
(ua) wK (wa) uJ
For = 0, the right-hand side must be zero. Also for = 0, either Eq. (2.55a) or (2.56a)
holds. Suppose Eq. (2.56a) holds, so that the term in square brackets on the right-hand
side in the above equation is not zero. Then we must have that B = 0, which from Eq.
(2.43) means that Hz = 0. Thus Eq. (2.56) corresponds to TM0m modes.
For the other case, substitute Eqs. (2.47) and (2.51) into Eq. (2.52):
0 = 1 B j J (ua) A uJ' (ua)
u2
a 1
8
+
1 jJ (ua) A w K' (wa)J (ua) B
w 2
a 2
K (wa)
With
k 2
1
= 21 and
k 2
2
= 22 rewrite this as
B =
ja 1
1
1
w
u 2 2
(k12J + k2
2K) A
where J and K are defined in Eq. (2.54). If for = 0 the term in square
brackets on the right-hand side is non-zero, that is, if Eq. (2.56a) does not hold,
then we must have that A = 0, which from Eq. (2.42) means that Ez = 0. Thus
Eq. (2.55) corresponds to TE0m modes.
2.17 From Eq. (2.23) we have
=
n2 n
2
12n12
2
=
1 1
2
n 2 2
n 2
1
<< 1 implies n1 n2
Thus using Eq. (2.46), which states that n2k = k2 k1 = n1k, we have
2 k 2
k 2 2 k 2 k 2 2
n
2 n
2 1 1
2.18 (a) From Eqs. (2.59) and (2.61) we have
M 2
2
2
a2 n12 n22
2
22
a2 NA
2
M 1/ 2 1000 1/ 2
0.85m a
30.25m
NA
2
0.22
9
Therefore, D = 2a =60.5 m
(b)
2 2
M 2 30.25m 2
414 0.2 1.32m 2
(c) At 1550 nm, M = 300
2.19 From Eq. (2.58),
V =
2 (25 m)
0.82 m
(1.48)2
2 1/
(1.46)
2
= 46.5
Using Eq. (2.61) M V2
/2 =1081 at 820 nm.
Similarly, M = 417 at 1320 nm and M = 303 at 1550 nm. From Eq. (2.72)
Pclad
P
total
4 3
M-1/2
=
4 100% 3 1080
= 4.1%
at 820 nm. Similarly, (Pclad/P)total = 6.6% at 1320 nm and 7.8% at 1550 nm.
2.20 (a) At 1320 nm we have from Eqs. (2.23) and (2.57) that V = 25 and M = 312.
(b) From Eq. (2.72) the power flow in the cladding is
7.5%. 2.21 (a) For single-mode operation, we need V 2.40.
Solving Eq. (2.58) for the core radius a
V 2 2 1/ 2 2.4 0(1.3 2m) m a = n n = = 6.55
1 2
2
2 2 (1.4 80) (1.4 78) 2 1/ 2
(b) From Eq. (2.23)
NA =
2 n
1
n 2 1/ 2
2
=
2
(1.480)
2
1/ 2
(1.478)
= 0.077
(c) From Eq. (2.23), NA = n sin A. When n = 1.0 then
10
A = arcsin
NA =
n
arcsin
0.077
1.0
= 4.4
2.22 n2 =
2
NA 2
= 2 2
= 1.427 n1 (1.458) (0.3)
a = V
= (1.30)(75)
= 52 m 2 NA
2(0.3)
2.23 For small values of we can write V 2 a
n1 2
For a = 5 m we have 0.002, so that at 0.82 m
V
2 (5
0.82
m)
m
1.45
2(0.002)
= 3.514
Thus the fiber is no longer single-mode. From Figs. 2.18 and 2.19 we see that
the LP01 and the LP11 modes exist in the fiber at 0.82 m.
2.25 From Eq. (2.77), Lp =
2
=
n y
n x
For Lp = 10 cm
For Lp = 2 m
Thus
ny - nx =
ny - nx =
1.3 10 6
10 1
m
1.3 106
2 m
m
m
= 1.310-5
= 6.510-7
6.510-7
ny - nx 1.310-5
2.26 We want to plot n(r) from n2 to n1. From Eq. (2.78)
n(r) = n1 1 2(r / a) 1 / 2
= 1.48 1 0.02(r / 25) 1 / 2
11
n2 is found from Eq. (2.79): n2 = n1(1 - ) =
1.465 2.27 From Eq. (2.81)
2 2 2
2an 2 M
1
a k n
2 2
1
where
=
n 1 n 2
n 1
= 0.0135
At = 820 nm, M = 543 and at = 1300 nm, M = 216.
For a step index fiber we can use Eq. (2.61)
M
step
V 2
2
=
1 2a 2
n2 n2
2 1 2
At = 820 nm, Mstep = 1078 and at = 1300 nm, Mstep = 429.
Alternatively, we can let in Eq. (2-81):
M
step =
2an1 2
=
1086 at 820 nm
432 at 1300 nm
2.28 Using Eq. (2.23) we have
(a) NA =
2 n
1
n 2 1/ 2
2
=
2
(1.60)
2 1/
(1.49)
2
= 0.58
2 2
1/ 2
= 0.39 (b) NA = (1.458) (1.405)
2.29 (a) From the Principle of the Conservation of Mass, the volume of a
preform rod section of length Lpreform and cross-sectional area A must equal the
volume of the fiber drawn from this section. The preform section of length
Lpreform is drawn into a fiber of length Lfiber in a time t. If S is the preform feed
speed, then Lpreform = St. Similarly, if s is the fiber drawing speed, then Lfiber = st.
Thus, if D and d are the preform and fiber diameters, respectively, then
Preform volume = Lpreform(D/2)2
= St (D/2)2
12
and
Equating these yields
D St 2
Fiber volume = Lfiber (d/2)2
= st (d/2)2
2 d 2 D 2
= st or s = S d
2
(b) S = s
d 2
D
= 1.2 m/s
0.125 mm
9 mm
2
= 1.39 cm/min
2.30 Consider the following geometries of the preform and its corresponding fiber:
25 m
R 4 mm
62.5 m
3 mm FIBER
PREFORM
We want to find the thickness of the deposited layer (3 mm - R). This can be
done by comparing the ratios of the preform core-to-cladding cross-sectional
areas and the fiber core-to-cladding cross-sectional areas:
A
A
preform core preform clad
=
A
A
fiber core
fiber clad
or 2 2
) (3 R 2 2
) (4 3
= (25)2
(62.5)2 (25)2
from which we have
R =
7(25)2
1/ 2
= 2.77 mm 9
2
2
(62.5) (25)
13
Thus, the thickness = 3 mm - 2.77 mm = 0.23 mm.
2.31 (a) The volume of a 1-km-long 50-m diameter fiber core is
V = r2
L = (2.510-3
cm)2
(105
cm) = 1.96 cm3
The mass M equals the density times the volume V:
M = V = (2.6 gm/cm3
)(1.96 cm3
) = 5.1 gm
(b) If R is the deposition rate, then the deposition time t is
t = M
= 5.1 gm
= 10.2 min
R
0.5 gm / min
2.32 Solving Eq. (2.82) for yields
K
2
=
where Y = for surface flaws. Y Thus
=
(20 N / mm 3 / 2 ) 2
(70 MN/ m 2 2
)
= 2.6010-4
mm = 0.26 m
2.33 (a) To find the time to failure, we substitute Eq. (2.82) into Eq. (2.86)
and integrate (assuming that is independent of time):
f
b / 2 d
i
t
= AYb
b
0
dt
which yields
1
1
or
t =
b 1f b / 2
1i b/ 2
= AYbbt
2
2 f b i
b)/ 2 2 b)/ 2 (2 (
(b 2)A(Y)
(b) Rewriting the above expression in terms of K instead of yields
14
2 2 b Kf 2 b
t = Ki
(b 2)A(Y) b
Y Y
2K
2 b b 2
b 2
i
if K
or b i << K f
(b 2)A(Y)
K 2 b
K 2 b
i f
15