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The Friis Transmission Formula
If we assume that the antennas are aligned for maximum transmission and
reception, then in free space,
PRX =GTXAePTX
4πr2
where Ae is the receiving aperture of the receiving antenna.
Since Ae =GRXλ2
4π
PRX = GTXGRXPTX
[
λ
4πr
]2
1 ENGN6521 / ENGN4521: Embedded Wireless L#10
Antenna Noise
Random noise comes from both objects and the sky (from space): E.G. The cosmicradiation background at 3oK.
Black body radiation => it must be there at finite temperature even in a vacuum!
This noise can be picked up by antennas. In a receiver it adds to the noise of the receiverelectronics.
PSD = No = KT where K = 1.38× 10−23J/oK and T is the absolute temperatureo−Kelvin.
The noise power is
PN = kTB
Such noise picked up by the antenna leads to the definition of antenna temperature.
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Link Budget: Friis transmission
Use the Friis transmission formula which applies to propagation between line of sightantennas:
PRX = GRXGTXPTXλ
(4πr)
2
where PTX and PRX are the transmit and received powers, GTX, GRX are the gains ofthe antennas at each end of the link.
Express in dBm (dB w.r.t 1 mW):
P (dBm) = 10 log10P (Watts)
.001
Express in dB with respect to 1 mW.. dBm
PRX(dBm) = PTX(dBm) + 10 log10GTX + 10 log10GRX +20 log10
(
λ
4πr
)
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Link Budget: Example
Determine required parabolic dish diameter of a 4 GHz earth station antenna if
its system temperature is 100k for an S/N ratio (SNR) of 20 dB, Bw 30MHz and
satellite transponder power of 5 Watts, dish diameter 2m
Some data...
SNR = PRX − PN . Here PRX will eventually mean at the very end of the receive chain.
Radius of geosynch. orbit = 42164kms
Radius of earth = 6371kms
Elevation od Geosynch. satellite = 35793 ≈ 36000kms
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Link Budget: Example
Determine required parabolic dish diameter of a 4 GHz earth station antenna if
its system temperature is 100k for an SNR of 20 dB, Bw 30MHz and satellite
transponder power of 5 Watts, dish diameter 2m
Pearth(dBm) = Psat(dBm) +Gsat +Gearth +20 log10 [λ
4π(36× 106)]
SNR = Psat(dBm)− PN +Gsat +Gearth +20 log10 [λ
4π(36× 106)] = 20dB
Gearth = (−Psat + 20+ Pn)−Gsat − 20log10[λ
4π(36× 106)]
where Gsat =4πAsat
λ2 = 35.4dB and Asat = πD2sat/8 = 1.6m2 is the satellite antenna aperture
(assuming 50% aperture efficiency).
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Link Budget: Example
Using noise and transmitted powers (dBm)
PN = 10 log10(KTB/.001) = −104dBm
PTX = 10 log10(5/.001) = 37dBm
we obtain Gearth = 39.3dB and Aearth = Gλ2
4πewhere e = 0.5 is the aperture efficiency,
Aearth = (10Gearth/10)λ2
4πe=> Dearth =
√
4Aearth
π
and Dearth = 3.12m.
6 ENGN6521 / ENGN4521: Embedded Wireless L#10
Satelllite Frequency Bands
7 ENGN6521 / ENGN4521: Embedded Wireless L#10
General Satellite System Block Diagram.
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Typical ground terminal
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Satellite Communications Systems (cont.)
The most desired frequency band for satellite communications is 6GHz on
the uplink (Earth to satellite) and 4GHz on the downlink (satellite to earth).
Why? In this range: 1) equipment is relatively inexpensive, 2) cosmic
noise is small and 3) rainfall does not appreciably attenuate the signals
(worse for higher f ⇒ smaller wavelength of order of size of raindrops.)
Unfortunately, these bands are already allocated to terrestrial microwave
radio relay links so the power density on Earth from satellites operating in
these bands is restricted .
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Satellite Communications Systems (cont.)
Also need to carefully place receivers for satellites in these bands so that
they do not receive interference signals from these microwave links.
In the 6GHz/4GHz band, satellites are assigned a spacing of 2.
Many satellite transponders do not demodulate the received signal before
retransmission. They simply amplify, down-convert (from say 6GHz to
4GHz) and then retransmit .
As technology allows, satellites will also process the incoming signals (e.g.
filter noise, reshape pulses) before retransmission. Will result in better
BER.
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Noise in Electronics - Johnson / Nyquist / thermal
Exists everywhere - even in a vacuum - The noise produced by thermal
equilibrium (as in Physics)
Noise power
Power(Watts) = kB T(oK) B(Hz)
where kB = 1.38× 10−23J/oK (Boltzmann’s constant)
Convert to dBm
P(dBm) = 10 log10kBTB
0.001
At T = 300oK and B = 7MHz(TV), P = −105dBm
Thermal noise power increases with bandwidth
12 ENGN6521 / ENGN4521: Embedded Wireless L#10
Noise in Electronics - Shot or Schottky noise
Arises from the discrete nature of charge carriers
Noise curremt (r.m.s.)
I2shot = 2qIdcB
where q = 1.6022× 10−19Coulomb (electronic charge)
Convert to power
Pshot = 10 log102RqIdcB
0.001
R = 50Ω, Idc = 1mA, Pshot = −100dBm.
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Man Made Noise
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Noise Performance of Amplifiers
When a signal of SNR, SNRi, with noise power Ni enters an amplifier
(any electronic device with gain) and exits with a new SNR, SNRo with
noise power No then we define the Noise Factor (F) of the network as,
F =SNRi
SNRo
Notice that SNRi is always > SNRo.
The Noise Figure is defined as,
NF = 10log10(F)
If the noise is only amplified then the NF is 0. In practice of course
amplifiers make things worse.
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The Noise Performance of Cascaded Amplifiers
The noise factor of cascaded amplifiers is given by,
FTOT = F1 +F2 − 1
G1+
F3 − 1
G1G2+ ...
where Gk are the power gains of the various amplifiers and Fk are the
noise factors
............
F1,G1 F2,G2 F3,G3 Fk,Gk
Provided that the amplifier gains are much larger than unity, the noise
factor (and therefore the noise figure) of a receiver chain is dominated by
that of the first amplifier.
16 ENGN6521 / ENGN4521: Embedded Wireless L#10
Noise Performance of Lossy Networks
If noise enters a lossy circuit then the NF is equal to the insertion loss (IL)
of the circuit.
NF = IL(dB)
Insertion Loss (IL) refers to that fraction of the signal power which is
dissipated in the network.
Insertion Loss (IL) is another name for the (power) transfer function
17 ENGN6521 / ENGN4521: Embedded Wireless L#10
Example Noise Power Calculation.
Consider the following receiver chain which is typical of that in a wireless
receiver.
The noise figure of the mixer and filter (both passive devices with the given
insertion losses) is 11dB.
Find the overall noise figure of the receiver
18 ENGN6521 / ENGN4521: Embedded Wireless L#10
Example Noise Power Calculation. (Contd)
The noise factor of the amplifier is 2 (=103/10).
The noise figure of the mixer and filter is 11 dB and so the noise factor is
12.6 (=1011/10). Thus,
FTOT = F1 +F2 − 1
G1= 2+ (12.6− 1)/10 = 3.16.
Finally we obtain
NF = 10log10(3.16) = 5dB.
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Receiver Noise Calculations
The thermal noise added to a signal when passing through a system is
given by,
No = kBTB
In dBm
No = 10log10kBTB
1× 10−3
If No and the NF are known, then the required input signal level for a given
output SNR can be calculated,
Si = NF +No + SNRo
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Receiver Noise Calculations (Example)
In the above example compute the required input signal level for a 10 dB
output SNR and a 1.25 MHz bandwidth.
No = 10log10(1.38× 10−23)(293)(1.25 × 106)
1.× 10−3= −113dBm
Therefore
Si = NF +No + SNRo = 5dB − 113dBm+10dBm = −98dBm
Notice that Johnson noise was assumed as the baseline input noise to the
receiver. This is rarely the case in practice
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Dealing with Noise
In telecommunications the effects of noise are mitigated by the choice of receivercomponents that have a low NF. That is: NF is the parameter to look for in activecomponent datasheets. Because it is that first amplifier in the receiver chain whichdetermines the noise figure, it is usually chosen to be a Low Noise Amplifier (LNA)(≪ 10dB NF).
To determine the sensitivity of a receiver in a particular application, one needs tomeasure the input noise from the antenna in situ and this will depend on thequietness of the site where the receiver is located. Site test .
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How to Measure Noise in Radio Receivers: SINAD (Signal to Noise And Distortion)
The method of measuring noise in arbitrary loads (e.g. antennas) and FM
receivers
Load
under
test
Coupler
1 kHz FM Modulated
carrier at RF frequency
FM Detector
I Khz
Notch filter
N(t) N(t) + W(t)
W(t)Audio amp
with AGC
RMS Volta meter
Galvanometer
set for 12 dB SINAD
26 ENGN6521 / ENGN4521: Embedded Wireless L#10
Spectrum Analyser Revision
LO Sweep generator is mixed with incoming signal
IF signal is passed through two filters.
IF filter : Resolution Bandwidth.
DC filter : Video Bandwidth.
Thus be wary when measuring the phase noise with a spectrum analyser.
27 ENGN6521 / ENGN4521: Embedded Wireless L#10
Transfer Function, Insertion Loss (Conversion Loss) and Attenuation.
The Transfer function of a four port network is the ratio of its output voltage Vo whenterminated (in Zo) to that when the network is replace by Zo.
Transfer function must be unity if the network is lossless.
Insertion loss is the same as the transfer function.
Attenuation only includes the loss from input to the output in terms of the voltage.
Transfer Function =2Vo
Zo
Attenuation =Vo
Vi
Transfer Function = Attenuation× (1 + ρ)
ρ =Zi − Zo
Zi + Zo
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