LinkBudget Analysis

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    ELE 492 – Fundamentals of Wireless Communica

    Place: E6

    Time: Wed. 13:00-16:00

    Textbooks:

    1. Molisch, Wireless Communications, 2nd Ed., Wiley

    2. Sklar, Digital Communications: Fundamentals and Applications, 2nd Ed., Prentice

    Assessment:

    1 Midterm Exam (40 %)

    1 Final Exam (60 %)

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

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    CommunicationsLink Analysis

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    dB in General

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    Power (dBW and dBm)

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    Power

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    Sensitivity level of GSM receiver: 6.3x10-14 W = -132 dBW or -102 dBm

    Bluetooth transmitter: 10 mW = -20dBW or 10dBm

    GSM mobile transmitter: 1 W = 0 dBW or 30 dBm

    GSM base station transmitter: 40 W = 16 dBW or 46 dBm

    Vacuum cleaner: 1600 W = 32 dBW or 62 dBm

    TV transmitter: 1000 kW ERP = 60 dBW or 90 dBm ERP

    Nuclear powerplant: 1200 MW = 91 dBW or 121 dBm

    ERP: effective radiated p

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    Amplification and Attenuation

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

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    Amplification and Attenuation

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    Noise Sources

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    Noise Sources

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    Communications Link

    The link contains/covers the entire communications path

    From the information source to the information sink

    Contains modulator/demodulator, encoder/decoder, pulse/matched filter, analog front e

    filters, etc), channel, etc.

    * Sklar, Digi

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

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    Link Budget Analysis

    Consists of the calculations and tabulation of the useful signal power and the interfpower present at the receiver.

    It is a balance sheet of gains and losses on the link

    Available power at the transmitter

    Tx + Rx antenna gains

    Propagation/channel losses

    Performance loss due to noise and natural/man-made interference

    Ultimately gives us the system requirements for a desirable performance of the link.

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

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    The Channel

    Channel is the propagating medium of electromagnetic path connecting the transmreceiver.

    Physically a channel can be For wired communications: Wire, coaxial cable, fiber optic cable,

    For wireless (RF) communications: empty space, waveguide, the atmosphere, earth’s surfcontaining «buildings, trees, vehicles, etc…»

    Free space: A channel free of all impairments to RFpropagation Absorption, reflection, refraction, diffraction

    Energy arriving at the receiver is only a function of the distance from the transmitter.

    We will consider the free space as the ideal channel!.

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

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    Error-Performance Degradation

    Main causes:

    1. Noise: thermal noise, impulsive noise, galactic noise, etc.

    2. Interference: Inter-Symbol Interference (ISI), Multi-User Interference (MUI), Other cominterference

    (Consider noise only for the time being.)

    Error performance depends on the received Signal-to-Noise Ratio per bit (SNR/bit

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Bit energy

    Noise PSD

    SNRAverage noise

    power

    Average signal

    power

    Bandwidth

    Rate

    LOSS HAPPENS HERE ! (HO

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    Sources of Signal Loss and Noise1. Bandlimiting Loss

    2. Intersymbol Interference(ISI)

    3. Local Oscillator PhaseNoise

    4. AM/PM Conversion(Amplitude

    variations)

    5. Limiter Loss orEnhancement

    12. Atmospheric Loss andNoise

    13. Space Loss

    14. Adjacent ChannelInterference

    15. Co-channel Interference

    16. Intermodulation Noise

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    6. Multiple-carrierIntermodulation

    Products (non-linear devices)

    7. Modulation Loss (messagecontent

    power)

    8. Antenna Efficiency

    9. Radome Loss and Noise

    10. Pointing Loss

    11. Polarization Loss

    17. Gand T

    18. Fe

    19. R

    20. Im

    21. ImSynch

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    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Sources of Signal Loss and Noise

    S

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    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Isotropic Antenna

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    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Dipole Antenna

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    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Dipole Antenna

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    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    dBi

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    Antenna Parameters

    Antenna

    (at the transmitter) is a transducer that converts electronic signals into electromagnetic f

    (at the receiver) converts electromagnetic fields into electronic signals.

    Hypothetical antenna: isotropic radiator

    Omnidirectional RF source: radiates uniformly over 4π steradians,

    Power density p(d) on the sphere of radius d is

    W/m2 (4πd2 = ?)

    Receiver side: In the far field (d >> λ)

    Ae: effective area of the an antenna

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Aer: receive antenna

    Aet: transmit antenna

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    Relation between the effective area (Ae) and the physical area (Ap) of an antenna

    efficiency parameter of an antenna η

    Dish antenna η = 0.55, horn antenna η = 0.75.

    Directive gain

    (If there is no loss or impedance mismatch, the antenna gain is equal to the directive

    Gain, which is the assumption here.)

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Antenna Parameters

    in a direction

    Power radiated

    by an isotropic

    radiator

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    Antenna Parameters

    Effective Radiated Power wrt. an isotropic radiator (EIRP) (Pt : transmitted power,Gt : gain the trans

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Both meters read

    the same power.

    For an isotropic

    radiatorFor an antenna

    With gain Gt

    ( Aer for

    is given

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    EIRP and the Link Budget

    EIRP = Transmit power (fed to the antenna) + antenna gain

    EIRP answers the questions:

    How much transmit power would we need to feed anisotropic antenna to obtain the same maximum on theradiated power?

    How strong is our radiation in the maximal direction of theantenna?

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

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    Antenna Parameters

    Antenna gain:

    Increasing frequency → Antenna gain increases

    Higher antenna dim.s→ more directional antenna

    → narrower beamwidth.

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    (G was given in slide 22.)

    h l ( )

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    Path loss (Free-space Loss)

    What is Ae for an isotropic receive antenna?

    Gr=1 →

    Received power Pr for an isotropic receive antenna (gain of the transmit antenna

    Path loss: attenuation of the received power

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    for the Tx antenna

    R i d Si l P

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    Received Signal Power (is frequency dependen

    Now, consider a receive antenna with gain Gr 

    Received signal power:

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Ae is a design param

    For fixed antennas (

    For fixed antennas (

    P h L

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    Path Loss (is frequency dependent)

    Path loss (free-space loss):

    One may express the received power in the logarithmic scale:

    It is sometimes useful to calculate Pr for «d = 1 m» and then scale d to find the act

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Geometric attenuation

    not freq. dependent

    Effective area

    freq. dependent

    ?

    Th l N i P

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    Thermal Noise Power

    Originates from the random motion of electrons in a conductor. PSD of this noise is hypothetically flat (constant) at all frequencies of interest.

    The maximum thermal noise power N that could be coupled observed at the front

    amplifier is

      κ : Boltzmann’s constant (1.38x10-23 W/K-Hz=-228.6 dBW/K-Hz)

    T: ambient temperature (o K)

    W: bandwidth (Hz)

    Max. single-sided noise PSD No available at the amplifier input is:

    and the noise power contained in a bandwidt

    No is dependent on the ambient noise (thermal noise) T . Similarly, the terminology effectivecan be use for noise with non-thermal origin (galactic, atmospheric, man-made noise, etc).

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    E /N

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    Eb/No SNR at the receiver input : C/N (Carrier-to-noise ratio)

    SNR at the predetection point: Pr/N (or S/N) ← this SNR term is used to calculate E

    For suppressed carrier modulation

    (What about a modulation scheme with carrier?)

    We have seen that , and , then for a digital receiver Pr/N

    (numerator: gains, denominator: losses).

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Receiver figure-of-merit

    Bit energy

    Noise PSD

    SNRAverage noise power

    Average received signal power Bandwidth

    Rate

    Li k M i

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    Link Margin

    Required SNR for a target BER is

    «to be on the safe side» add a couple of dBs for thereceived SNR

    «safety margin» -> link margin

    Remember that , then

    or

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    Li k M i

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    Link Margin

    Read Sections 5.4.3 and 5.4.4 from Sklar (discussion about link margin, satellite coavailability).

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Noise Figure

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    Noise Figure

    Noise figure, F, relates the SNR at the input of a network to the SNR at the output o

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Noise Figure

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    Noise Figure

    Si : signal power at the amplifier input port

    Ni : noise power at the amplifier input port

    Na: noise power introduced at the amplifier

    Nai : amplifier noise referred to the input port

    G: amplifier gain.

    ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    A reference for Ni  is when T 0 = 290oK (refe

    No = κ T o = 1.38 x 10-23 x 290 = 4.00 x 10-21 W/

    No = - 204 dBW/Hz @ T 0 = 290oK 

    An amplifier amp

    but also amplifies

    and also introduc

    *

    Spring 2015

    (Typical valu

    Noise Temperature

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    Noise Temperature

    ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

     T 0 = 290oK : reference temperature, T R: effective noise temperature of the receive

    For the output of an amplifier, we can write the output noise power as

    T g: temperature of the source.

    Spring 2015

    (What percentag

    (Ni @ T 0)(Ni @ T R)

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    Line Noise

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    Line Noise

    Let all components be at temperature T g.

    There is thermal equilibrium -> no current flows due to noise.

    Assume that the impedances of the input and output of the network is matched with tthe load.

    The total output noise power Nout flowing from the network to the load:

    Ngo: noise at the output due to the source

     GNLi : noise at the output due to the lossy network (NLi : network noise relative to its inp

    Due to thermal equilibrium, noise power of the load is also equal to κ T gW.

    ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONSSpring 2015

    Line Noise

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    Line Noise

     NLi : network noise relative to its input:

    Effective noise temperature of the line, T L, is

    If the ambient temperature is T g = T 0 = 290oK (above derivation assumes line temp

    Noise figure for a lossy line is

    Then the output noise power is (see pg. 34)

    ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONSSpring 2015

    {

    Line Loss

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    Line Loss

    Example:

    T0 = 290oK

    Tg = 1450oK

    Si = 100 pW

    W = 1 GHz

    L=2

    Calculate (SNR)in,

    (SNR)out and

    TL.

    ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONSSpring 2015

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    System Effective Temperature

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    System Effective Temperature

    Apart from the transmission line and pre-amplifier, external noise sources are also

    natural noise sources: lightning, atmospheric noise, cosmic noise, thermal radiation from

    man-made noise sources: automobile ignition, electrical machinery, other radio signals, e

    They are represented by antenna temperature T  A (κ T  AW).

    System temperature is

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    System Performance (w/o LNA)

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    System Performance (w/o LNA)

    Example: Receiver without a LNA preamplifier (no line loss)

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    From source From front-end

    System Performance (w LNA)

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    System Performance (w LNA)

    Example: Receiver with a LNA preamplifier (no line loss)

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    From source From front-end

    Sky Noise Temperature

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    Sky Noise Temperature

    When the antenna points towards the sky:

    Up to 1 GHz, galactic noise is dominant.

    After 10 GHz atmospheric noise is dominant.

    There is an available window in between with low

    natural noise.

    (Observe variation wrt. elevation.)

    (Study Example 5.7 and Sections 5.4.4 and 5.5.6.1 for satellite comm.s)

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS

    Sample Link Analysis

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    Sample Link Analysis

    Brackets: () loss

    No brackets: gain

    Box: subtotalsDouble box: link margin.

    Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS