3F4 Power and Energy Spectral Density

12
3F4 Power and Energy Spectral Density Dr. I. J. Wassell

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3F4 Power and Energy Spectral Density. Dr. I. J. Wassell. Power and Energy Spectral Density. The power spectral density (PSD) S x ( w ) for a signal is a measure of its power distribution as a function of frequency - PowerPoint PPT Presentation

Transcript of 3F4 Power and Energy Spectral Density

Page 1: 3F4 Power and Energy Spectral Density

3F4 Power and Energy Spectral Density

Dr. I. J. Wassell

Page 2: 3F4 Power and Energy Spectral Density

Power and Energy Spectral Density

• The power spectral density (PSD) Sx() for a signal is a measure of its power distribution as a function of frequency

• It is a useful concept which allows us to determine the bandwidth required of a transmission system

• We will now present some basic results which will be employed later on

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PSD

• Consider a signal x(t) with Fourier Transform (FT) X()

dtetxX tj )()(

• We wish to find the energy and power distribution of x(t) as a function of frequency

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Deterministic Signals• If x(t) is the voltage across a R=1 resistor,

the instantaneous power is,2

2

))(())((

txR

tx

• Thus the total energy in x(t) is,

dttx 2)(Energy

• From Parseval’s Theorem,

dfX2

)(Energy

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Deterministic Signals• So,

dfX2

)(Energy

dffE

dffX

)2(

)2(2

Where E(2f) is termed the Energy Density Spectrum (EDS), since the energy of x(t) in the range fo to fo+fo is,

oo ffE )2(

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Deterministic Signals• For communications signals, the energy is

effectively infinite (the signals are of unlimited duration), so we usually work with Power quantities

• We find the average power by averaging over time

2

2

2))((1lim

power AverageT

T

T dttxTT

Where xT(t) is the same as x(t), but truncated to zero outside the time window -T/2 to T/2

• Using Parseval as before we obtain,

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Deterministic Signals

2

2

2))((1lim

power AverageT

T

T dttxTT

dffS

dfT

fX

T

dffXTT

x

T

T

)2(

)2(lim

)2(1lim

2

2

Where Sx() is the Power Spectral Density (PSD)

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PSD

T

X

TS T

x

2)(lim

)(

The power dissipated in the range fo to fo+fo is,

oox ffS )2(

And Sx(.) has units Watts/Hz

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Wiener-Khintchine Theorem• It can be shown that the PSD is also given by

the FT of the autocorrelation function (ACF), rxx(),

derS jxxx )()(

Where,

2

2

)()(1lim

)(

T

Txx dttxtx

TTr

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Random Signals

• The previous results apply to deterministic signals

• In general, we deal with random signals, eg the transmitted PAM signal is random because the symbols (ak) take values at random

• Fortunately, our earlier results can be extended to cover random signals by the inclusion of an extra averaging or expectation step, over all possible values of the random signal x(t)

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PSD, random signals

• The W-K result holds for random signals, choosing for x(t) any randomly selected realisation of the signal

T

XE

TS T

x

])([lim)(

2

Where E[.] is the expectation operator

Note: Only applies for ergodic signals where the time averages are the same as the corresponding ensemble averages

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Linear Systems and Power Spectra• Passing xT(t) through a linear filter H() gives

the output spectrum,)()()( TT XHY

• Hence, the output PSD is,

T

XHE

TT

YE

TS TT

y

])()([lim])([lim)(

22

T

XE

THS T

y

])([lim)()(

22

)()()(2 xy SHS