E4702 HW#1 solutions - Columbia Universityegc/e4702_HW1.pdfE4702 HW#1 solutions by Anmo Kim...
Transcript of E4702 HW#1 solutions - Columbia Universityegc/e4702_HW1.pdfE4702 HW#1 solutions by Anmo Kim...
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E4702 HW#1 solutionsby Anmo Kim ([email protected])
office hour: 2-3PM TUE&THR (1247 Mudd)
1. (P1.15) A running integrator is defined by
y(t) = t
tTx()d (1)
where x(t) is the input, y(t) is the output, and T is the integration period. Both x(t) and y(t) are samplefunctions of stationary processes X(t) and Y (t), respectively. Show that the power spectral density of theintegrator output is related to that of the integrator input by
SY (f) = T 2sinc2(fT )SX(f) (2)
(Solution)
The relation between SY (f) and SX(f) can be described by (1.58) in Haykins.
SY (f) = |H(f)|2SX(f)
Thus, we need to show that |H(f)|2 = T 2sinc2(fT ).The impulse response h(t) can be directly obtained from (1) by giving the impulse function, (t), as an input.
h(t) = { 1, 0 t T0, otherwise
By the Fourier transform,
H(f) = T
0
1 ej2ftdt
=1
j2f(ej2fT 1)
=1
2f [sin 2fT + j(cos 2fT 1)]
Then,
|H(f)|2 = 1(2f)2
[(sin 2fT )2 + (cos 2fT 1)2]
=1
(2f)2 [2 2 cos 2fT ]
=4 sin2 fT
(2f)2
= T 2sinc2(fT )
Thus,SY (f) = T 2sinc2(fT )SX(f)
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2. (P1.16) A zero-mean stationary process X(t) is applied to a linear filter whose impulse response is defined bya truncated exponential:
h(t) = { aeat, 0 t T0, otherwise
Show that the power spectral density of the filter output Y (t) is
SY (f) =a2
a2 + 42f2(1 2 exp(aT ) cos(2fT ) + exp(2aT ))SX(f)
where SX(f) is the power spectral density of the filter input.
(Solution)
Since X(t) is a stationary process, then as in (P1.15), SY (f) can be described by the following equation.
SY (f) = |H(f)|2SX(f)
The Fourier transform of the given h(t) is
H(f) =
h(t)ej2ftdt
= T
0
ae(a+j2f)tdt
= aa + j2f
[e(a+j2f)T 1
]
Then,
|H(f)|2 = H(f)H(f)
={ a
a + j2f[e(a+j2f)T 1
]}{ a
a j2f [e(aj2f)T 1
]}
=a2
a2 + 42f2 [1 2eaT cos(2fT ) + e2aT ]
Thus,
SY (f) =a2
a2 + 42f2(1 2 exp(aT ) cos(2fT ) + exp(2aT ))SX(f)
3. (P1.17) The output of an oscillator is described by
X(t) = A cos(2Ft)where A is a constant, and F and are independent random variables. The probability density function of is defined by
f() = {12 , 0 20, otherwise
Find the power spectral density of X(t) in terms of the probability density function of the frequency F . Whathappens to this power spectral density when the frequency assumes a constant value?
(Solution)
Because and F are independent, the joint probability density function becomes:
f,F (, x) = f() fF (x)
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Then, autocorrelation function of X(t) becomes:
RX(t, u) = E[X(t)X(u)]
=
x
f,F (, x)X(t)X(u)ddx
=
20
12
fF (x)X(t)X(u)ddx
=12
fF (x) 2
0
A2 cos(2xt ) cos(2xu )ddx
=A2
2
fF (x)12
20
[cos(2x(t + u) 2) + cos(2x(t u))] ddx
=A2
2
fF (x) cos(2x(t u))dx
Let = t u,RX() =
A2
2
fF (x) cos(2x)dx (3)
And RX() can be represented as a Fourier transform pair of power spectral density, SX(x):
RX() =
SX(x) exp(j2x)dx (4)
Since RX() is a real and even function,
RX() =
SX(x) cos(2x)dx (5)
From the similarity between (3) and (5), we can get SX(x) without calculating the Fourier transform ofRX() directly.
SX(x) =A2
2fF (x)
If the frequency x is a constant value, x0, fF (x) = 12(x x0) + 12(x + x0). Thus, SX(x) becomes:
SX(x) =A2
4(x x0) + A
2
4(x + x0)
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