LinkBudget Analysis
Transcript of 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
Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS
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
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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
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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.
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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!.
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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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Isotropic Antenna
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Dipole Antenna
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Dipole Antenna
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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
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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?
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Antenna Parameters
Antenna gain:
Increasing frequency → Antenna gain increases
Higher antenna dim.s→ more directional antenna
→ narrower beamwidth.
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(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
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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:
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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).
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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
Spring 2015 ELE 492 – FUNDAMENTALS OF WIRELESS COMMUNICATIONS
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
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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
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(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.
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(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.
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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.
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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)
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Sample Link Analysis
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Sample Link Analysis
Brackets: () loss
No brackets: gain
Box: subtotalsDouble box: link margin.
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