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    EE 3323

    Principles of CommunicationSystems

    Section 8.2Noise

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    Communication Systems

    A typical (simplified) communication system isillustrated below.

    Transmitter TransmissionMedium Receiverx(t)

    n(t)

    J(t)y(t)

    J(t) + n(t)

    The message signalx(t) is applied to a Transmitter

    here the signal is perhaps conditioned and used toodulate a carrier signal. The modulated signal

    J(t) is transmitted through a medium ( ree space,coaxial cable, iber optic cable, etc.).

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    Communication Systems

    In the course o transmission, the modulated signalis corrupted by the addition o noise. The noise

    corrupted, modulated signal is applied to a Receiver

    that Demodulates the signal and perhaps conditions

    the resulting signal. The outputy(t) is related to theinputx(t) in a predictable ay. O ten the desire is

    ory(t) to be a replica o x(t).

    model is need to access the e ects o noise at theinput o the receiver and at the output o the

    receiver.

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    White Gaussian Noise

    The irst model or Noise is White, Gaussian Noise.

    This model is termed White because the Po er

    Spectral Density contains all requencies equally.

    This is an analogy to White Light, that contains allvisible avelengths.

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    White Gaussian Noise

    This model is termed Gaussian because theinstantaneous value o the noise signal is a Gaussian

    distributed random variable completely described by

    the mean and variance. This is a convenient

    distribution to use. It adequately represents manynoise sources (due to the central limit theorem).

    The mean squared represents the DC po er o the

    noise, and the variance represents the total average

    po er in the noise.

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    White Gaussian Noise

    The Po er Spectral density o White GaussianNoise is depicted belo .

    -8 -7 -6 -5 -4 -3 -2 -1 0 1 2 3 4 5 6 7 8

    Snn ( f )

    f

    N0

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    White Gaussian Noise

    Notice that this Po er Spectral Density implies anoise source o in inite po er. The one-hal actor

    is a convention that ill make sense hen Band-

    limited noise is discussed.

    The utocorrelation o Gaussian White Noise is

    Rnn

    (X) = F1 {Snn

    ( f)}

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    White Gaussian Noise

    Rnn(X) N02 H(X)

    -8 -7 -6 -5 -4 -3 -2 -1 0 1 2 3 4 5 6 7 8

    R nn (X)

    X

    N0

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    White Gaussian Noise

    Observe that this Autocorrelation implies aninfinitely rapid changing noise signal. The White

    oise signal is un-correlated with itself after the

    most minute time shift. Obviously such a noise

    model does not reflect any physical process. Amore realistic noise model follows.

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    Band-limited Noise

    Consider passing White aussian oise through anideal Low-pass Filter of bandwidth B. The ower

    pectral ensity of such oise is shown below.

    -8 -6 -4 -2 0 2 4 6 8

    Snn ( f )

    f

    N0

    BB

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    Band-limited Noise

    Snn( f) = N0

    2rect

    f2B

    The average po er in this noise signal is

    Pn = N0B

    The Noise Po er is directly proportional to the

    band idth o the lo -pass ilter.

    The utocorrelation is

    Rnn(X) =N0

    22B sinc(2BX)

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    Band-limited Noise

    Rnn(X) N0B sinc

    X1/2B

    -8 -7 -6 -5 -4 -3 -2 -1 0 1 2 3 4 5 6 7 8

    R nn (X)

    X

    N0B

    1/2B

    1/2B

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    Thermal Noise

    The thermal noise in a resistor (due to randommotion of the electrons in the resistor) is described

    by the following ower pectral ensity.

    Snn( f)2 Rh

    | |f

    exp

    h| |f

    kT 1

    where:

    Value of the resistor (Ohms)h lanks Constant 6.625 v 10

    34(joule sec)

    k oltzmanns constant 1.38 v 1023

    (joules / K)

    T Temperature of the resistor in K13

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    Thermal Noise

    103

    106

    109

    1012

    1015

    103

    106

    109

    1012

    1015

    f

    Snn (f )

    This is essentially constant for frequencies typically

    used in electronic systems.

    Snn( f) 2 k TR

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    Thermal Noise

    A noise model for a resistor is:

    Noiseless

    R

    nn( f) 2 k TR

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    Thermal Noise

    Example: Find the RM voltage due to thermalnoise that may be measured in the following circuit

    with R 1 k;, C 1 QF and T 300 K.

    Noiseless

    R

    nn( f) 2kTR

    R C Cv(t)

    v(t)

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    Thermal Noise

    The RC circuit forms a filter with transfer function

    H( f)1

    1 +j 2TRC f

    The magnitude squared of the transfer function is

    | |H( f)2

    1

    1 + (2TRC)2 f2

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    Thermal Noise

    H( f) 2 = 11 (2TR )2 f2

    f

    H( f ) 2

    0 101

    102

    103

    101

    102

    103

    B NB N

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    Thermal Noise

    The po er spectral density at the terminals due tothermal noise is

    Syy( f) = Snn( f) H( f)2

    Syy( f) =2 k R1

    1 (2TR )2 f2

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    Thermal Noise

    And the total noise po er appearing at the terminalsis

    Py = 20

    g

    Syy ( f) df

    Py = 20

    g

    2 k R 11 (2TR )2 f2df

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    Thermal Noise

    Using the inde inite integral

    g

    g

    dx

    a2 b

    2x

    2 =1

    abtan

    1

    bx

    a

    Py = 4 k R1

    2TRtan

    1(2TR f)

    g

    0

    Py = 4 k

    R

    1

    2TR

    T

    2

    Py =k

    C

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    Thermal Noise

    The S voltage appearing at the terminals is

    Vrms =k

    C

    or the speci ic values given above

    Vrms =1.38

    v10

    23(300)

    1 v 10 6

    Vrms = 0.06 QV22

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    Equivalent Noise Bandwidth

    Assuming the input to a ilter is Gaussian White Noise ith constant noise po erN0/2, and the

    trans er unction o the ilter is kno n, e ish to

    de ine an ideal ilter that passes the equivalent noise

    po er.

    f

    H( f )2

    0 101

    102

    103

    101

    102

    103

    B NB N

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    Equivalent Noise Bandwidth

    Py = 2

    0

    g

    N0

    2 H( f) 2df= N0 H(0)

    2BN

    BN =

    20

    g

    N0

    2 H( f)2

    df

    N0 H(0)2

    BN =

    0

    g

    H( f) 2df

    H(0)2

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    Equivalent Noise Bandwidth

    If the filter is a simple lo -pass C filter as sho nabove,

    H

    (f

    )

    2

    =

    1

    1 (2TRC)2 f2

    and

    BN =

    0

    g

    1

    1 (2TRC)2 f2df

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    Equivalent Noise Bandwidth

    BN =1

    2TRCtan

    1(2TRC f)

    g

    0

    BN =

    1

    2TRC

    T

    2

    BN =1

    4RC

    is the equivalent noise band idth of the C lo -

    pass filter.

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    BandpassWhite Noise

    Consider passing White Gaussian Noise through aBand-pass ilter ith band idth B. The Po er

    Spectral Density of the filtered noise is:

    -8 -7 -6 -5 -4 -3 -2 -1 0 1 2 3 4 5 6 7 8

    Snn ( f )

    f

    N0

    B

    f0f0

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    BandpassWhite Noise

    Snn( f) = N02rect

    fB

    * [H( ff0) H( f+f0)]

    The total average po er is

    P= N0B

    Again, the average po er is proportional to the

    band idth of the filter.

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    BandpassWhite Noise

    The Autocorrelation is

    Rnn() =N0

    2B sinc(BX) 2 cos(2Tf0X)

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    BandpassWhite Noise

    Rnn() = N0B sinc X1/B

    cos(2Tf0X)

    R nn (X)

    X

    N0B

    1/B

    1

    /f0

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    Noise Power ofBand-limitedWhite Noise

    The Po er Spectral Density of Band-limited Noiseis often defined using an Ideal o -pass filter as

    illustrated belo .

    -8 -6 -4 -2 0 2 4 6 8

    Snn ( f )

    f

    N0

    BB

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    Noise Power ofBand-limitedWhite Noise

    The average po er in this noise signal is

    Pn = N0B

    easured in Watts across a one-ohm resistance. Ingeneral, the noise voltage ill be measured across a

    resistance as follo s.

    n(t)

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    Noise Power ofBand-limitedWhite Noise

    For such a Band-limited noise source, the averagepo er dissipated in the resistance is

    n2(t) = N0BR

    So if 100 mW of Noise, Band-limited to 1000Hz is

    dissipated across a 50; resistance, the Noise po eris

    N0 =n2(t)

    BR=

    .1

    1000(50)= 2 QW/Hz

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    Narrowband Noise

    If Gaussian White noise is passed through a band-pass filter here the bandwidth of the filter is small

    compared to the centerfrequency, it is possible to

    develop a time-representation of the random noise

    signal.

    This effect is illustrated below.

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    Narrowband Noise

    0 0.02 0.04 0.06 0.08 0.1-4

    -2

    0

    2

    4

    Time ( )

    n(t)

    Gaussian White Noise signal

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    Narrowband Noise

    Autocorrelation of aussian White Noise ignal

    -0.1 -0.05 0 0.05 0.1-0.5

    0

    0.5

    1

    1.5

    Time ( )

    Rx

    x(tau)

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    Narrowband Noise

    Power pectral ensity of aussian White Noise

    ignal

    -1000 -500 0 500 10000

    1

    2

    3

    4

    5x 10

    -3

    Frequency ( z)

    xx(f)

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    Narrowband Noise

    This aussian White Noise is passed through aand-pass Filter as illustrated below.

    and-pass Filter

    Center Frequency =f0Bandwidth = B

    nw(t) n(t)

    For this examplef0 = 200 z andB = 40 z.

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    Narrowband Noise

    Narrow and Noise

    0 0.02 0.04 0.06 0.08 0.1-1

    -0.5

    0

    0.5

    1

    Time ( )

    n

    bn(t)

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    Narrowband Noise

    The narrow-band noise signal appears to be asinusoid with a slowly varying amplitude and

    phase.

    The nominal frequency is the same as the centerfrequency of the band-pass filter.

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    Narrowband Noise

    -0.1 -0.05 0 0.05 0.1-0.05

    0

    0.05

    Time ( )

    Rxx(tau)

    Autocorrelation ofNarrowband Noise

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    Narrowband Noise

    Power pectral ensity ofNarrowband Noise

    -1000 -500 0 500 10000

    1

    2

    3

    4x 10-6

    Frequency (k z)

    xx(f)

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    Narrowband Noise

    This Pow

    er Spectral Density is relatively narrow

    (looking somewhat like a delta function). Perhaps a

    time representation is available.

    A phasor representation of narrowband noise is asfollows

    nc(t)

    ns(t)

    an

    Un

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    Narrowband Noise

    n(t) = [ ]nc(t)+jns(t) (j Tf0t)

    n(t) = [ ]nc(t)+jns(t) [ ](2Tf0t)+j (2Tf0t)

    n(t) =

    nc(t) (2Tf0t)+jnc(t) (2Tf0t)

    +jns(t) (2Tf0t)+jjns(t) (2Tf0t)

    n(t) = nc(t) (2Tf0t) ns(t) (2Tf0t)

    wherenc(t) ns(t) reran omnoise rocesses.

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    Narrowband Noise

    Both nc(t) and ns(t) are low-pass (relatively low-frequency) random signals.

    nc(t) in-phase component

    ns(t) quadrature component

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    Narrowband Noise

    An alternative expression is

    foun

    dby letting

    nc(t) = a(t)cos[J(t)]

    ns(t) = a(t)sin[J(t)]

    n(t) = a(t)cos[J(t)]cos(2Tf0t) a(t)sin[J(t)]sin(2Tf0t)

    n(t) =

    1

    2a(t) cos[J(t) + 2Tf0t] +1

    2a(t) cos[J(t) 2Tf0t]

    1

    2a(t) cos[J(t) 2Tf0t] + cos[J(t) + 2Tf0t]

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    Narrowband Noise

    n(t) a(t) cos[2Tf0t+ J(t)]

    where a(t) is a randomly varying amplitude and J(t)is a randomly varying phase angle.

    a(t) nc2(t) + ns

    2(t)

    J(t) tan 1

    ns(t)

    nc(t)

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    Narrowband Noise

    The random amplitude is described by a RayleighPDF

    fA(a)a

    2TWA2 exp

    a2

    WA2 , au 0.

    where WA2 is the RM power in the narrow-bandnoise signal.

    0

    0.8

    -1 0 1 2 3 4 5a

    fA (a ) WA 1

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    Narrowband Noise

    The random phase angle is described by a uniformdistribution

    f*(J)1

    2T, 0 eJ 2T

    0

    0.1

    0.2

    -2 0 2 4 6 8J

    f*

    (J)

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    Signal to Noise Ratio

    Recall the simplified communication system shownbelow.

    TransmitterTransmission

    Medium Receiverx(t)

    n(t)

    J(t) y(t)J(t) + n(t)

    Sin ,Nin Sout ,Nout

    The signal at the input of the receiver is corruptedby noise. We make these assumptions about the

    noise.

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    Signal to Noise Ratio

    1. The noise is zero-mean, aussian distributed,white noise with power spectral density

    Snn( f)N0

    2

    2. The noise is uncorrelated with the modulated

    signal J(t).

    3. The noise is additive.

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    Signal to Noise Ratio

    Under these conditions, the signal power input to thereceiver is

    E{ }[ ]J(t) + n(t) 2 E{ }J2 (t) + E{ }2J(t)n(t)

    + E{ }n2(t)

    ince the noise is zero-mean

    E{ }[ ]J(t) + n(t)2

    E{ }J2

    (t) + E{ }n2

    (t)

    E{ }[ ]J(t) + n(t) 2 Sin +Nin

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    Signal to Noise Ratio

    The quality of

    the signal can be measured

    byforming the signal-to-noise ratio

    S

    N

    in

    =Sin

    Nin

    =E{ }J2 (t)

    E{ }n2

    (t)

    The larger the signal-to-noise ratio, the better the

    received signal quality

    The signal-to-noise ratio is often measured indecibels

    S

    N

    in dB

    = 10 log10

    Sin

    Nin

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    Signal to Noise Ratio

    In like manner, the signal o

    fthe receive

    dmessage isis given by

    S

    N out =

    Sout

    Nout =

    E{ }y2(t)

    E{ }n2(t)

    S

    N

    out dB

    = 10 log10

    Sout

    Nout

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