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University of California Los AngelesComputer Science Department
DIMENSIONING
Application
Presentation Application
Session
Transport Transport
Network Internet
Data Link Network Interface
Physical Layer Physical
Winter 2002 CS216 - Satellite Networks P08/2
University of California Los AngelesComputer Science Department
Link Dimensioning
Titolo diagramma
AntennaParameters
NoisePower
Influenceof the propagation
medium
Signalto noise
ratio
SystemImplicationsShadowing
Multiptath Fading
LINK ANALYSIS
It concerns the trasmission of radio waves between twoearth stations, one transmitting and one receiving, viasatellite. In this context, the link consists of twosegments: the uplink from the transmitting earth stationto the satellite and the downnlink from satellite to thereceiving earth station.
Winter 2002 CS216 - Satellite Networks P08/3
University of California Los AngelesComputer Science Department
Characteristic Parameters of an Antenna (1)• Gain is the ratio between the power radiated per unit solid angle by an
antenna in a given direction and the power radiated per unit solid angleby an isotropic antenna fed with the same power. It is given by:
Gmax = ( 4π / λ2 ) Aeff
λ= c / f wavelenght of the electromagnetic wave,c velocity of the light,f frequency of the electromagnetic wave,Aeff =η A effective aperture area for an antenna with a circular
aperture of diameter D and geometric surface A=π D2/4η efficiency of antenna (tipically 0.5-0.65).
Gmax = η (πD/λ)2 =η(πD f/c)2
• The efficiency of antenna is the product of several factors:the illumination law
the spill-over lossthe surface impairmentsresistive and mismatch losses
η = η i ∗ ηs ∗ ηf ∗ ηz
Winter 2002 CS216 - Satellite Networks P08/4
University of California Los AngelesComputer Science Department
Characteristic Parameters of an Antenna (2)
• The Radiation pattern indicates the variations of gain with direction.For an antenna with a circular aperture or reflector this pattern hasrotational symmetry. The main lobe contains the direction of themaximum radiation while side lobes should be kept to a minimum.
• The Angular Beamwidth is the angle by the directionscorresponding to a given gain fallout with respect to the maximumvalue.The 3 dB beamwidth is often used, it correspondes to theangle between the directions in wich the gain falls to half itsmaximum value.
• For uniform illumination the angle is 58.5°, with non u. ill. The angleincreases and the value commonly used is 70° wich leads thefollowing expression
θ3dB= 70 (λ/D) = 70(c/f D)• Thus Gmax=η (π 70 /θ)2
Winter 2002 CS216 - Satellite Networks P08/5
University of California Los AngelesComputer Science Department
Antenna radiation pattern characteristics
Dθ
main lobe
side lobes
dish
θ3dB
GmaxGmax-3dB
θ3dBθ
Gmax
Gmax-3dB
Gmax-30dB
Winter 2002 CS216 - Satellite Networks P08/6
University of California Los AngelesComputer Science Department
Teta 3dB
0
1
2
3
4
5
6
7
8
9
10
0,1 1 10
Antenna diameter (m)
Tet
a (d
egre
es)
'4 GHz''6 GHz''12 GHz''14 GHz''20 GHz''30 GHz'
Winter 2002 CS216 - Satellite Networks P08/7
University of California Los AngelesComputer Science Department
Characteristic Parameters of an Antenna (3)
• Polarisation , convention isdefined by the direction ofthe electric field. In generalthe direction of electric fieldis not fixed during oneperiod, the extremity of thevector of e.f. describes anellip s e . Polarisation ischaracterized by:
Direction of rotation
Axial ratio = E max / E min
Inclination of ellipse
• Two waves are in orthogonalpolarisation if their electricfields describe identicalellipses in opposite directions.
• Orthogonal polarisations:- Circular: RHCP - LHCP
- Linerar: HP - VP
Winter 2002 CS216 - Satellite Networks P08/8
University of California Los AngelesComputer Science Department
Emitted Power• The power radiated per unit solid angle by an isotropic
antenna fed from a radio-frequency source of powerPt = Pt/4π (W/steradian)
for a gain Gt any antenna radiates a power per unitsolid angle equal to:
Gt Pt / 4πThe product Gt Pt is called EIRP (Effective IsotropicRadiated Power)
Winter 2002 CS216 - Satellite Networks P08/9
University of California Los AngelesComputer Science Department
Received Power
• A surface of area A located at a distance R from thetransmitting antenna subtends a solid angle A/R2 andreceives a power:
Pr= (PtGt/4π)(A/R2) = FA (W) F: power flux density (W/m2)• A receiving antenna of effective aperture area Areff located
at distance R from the transmitting antenna receives thepower
Pr = FAreff =(PtGt/4πR2)Areff
with Areff=Gr/(4π/λ2)
Pr= PtGtGr/Lfs
Lfs=(4πR/λ)2 free space loss(ratio between received and transmitted power function of f)
Winter 2002 CS216 - Satellite Networks P08/10
University of California Los AngelesComputer Science Department
Other losses
• Transmitting and receiving losses due to waveguides
• Pointing losses
• Atmospheric losses (when applicable)– rain
– clouds
– gas (water vapour and oxygen)
– tropospheric scintillation
• Polarization losses
• Mobile channel losses (when applicable)
L = Ltx + Lrx + Lp + La + Lpol + Lm
Winter 2002 CS216 - Satellite Networks P08/11
University of California Los AngelesComputer Science Department
Pointing error
• The movement of the satellite causes the misalignment ofthe boresights of the two antennas
• It can be evaluated with the following formula:
ε θθ
=
12
3
2
dB
θ
Winter 2002 CS216 - Satellite Networks P08/12
University of California Los AngelesComputer Science Department
Pointing error plot
0
5 0
100
150
200
250
300
350
400
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
Teta (degrees)
Poi
ntin
g er
ror
(dB
)
'4 GHz'
'6 GHz'
'12 GHz'
'14 GHz'
'20 GHz'
'30 GHz'
Winter 2002 CS216 - Satellite Networks P08/13
University of California Los AngelesComputer Science Department
Signal to Noise Ratio (C/N)
• C = EIRP - L + GR
• Thermal noise characterized by power spectral density
N0 = k T– k : Boltzman constant = 1.38·10-23 Ws/K = -228.6 dBWs/K
– T effective noise temperature
T = Ta + Tr
– Ta: receiving antenna noise temperature
– Tr: effective noise temperature of the receiver
80Earth terminal 10° elevation
3-10Earth terminal 90° elevation
290Satellite
Noise Temperature (K)Antenna
Winter 2002 CS216 - Satellite Networks P08/14
University of California Los AngelesComputer Science Department
C/N & Eb/N0
If noise figure Nr of the receiver is provided
Tr = (10Nr/10 - 1)·290 K
G/T figure of merit
C/N0 = Pt + Gt - L + GR - k - T = EIRP - L + G/T - k dBHz
C/N = C/(N0·BR)
BR noise equivalent bandwidth
Eb/N0 = (C/N0)· Tb = (C/N0) ·(1/ Rb)
Eb/N0 = C/N0 - Rb = EIRP - L + G/T - k - Rb
CN
CkT
P GL
GkT
EIRPL
G Tk
t t R
0
= = ⋅ = ⋅ /
Winter 2002 CS216 - Satellite Networks P08/15
University of California Los AngelesComputer Science Department
Example 1: The uplink• Antenna of an earth station with diameter D = 4m• Antenna is fed with a power P = 100 W , 20 dBW, at a frequency f =14 GHz• Antenna radiates this power towards a GEO satellite at a distance of 40000
km on the axis of antenna• The beam of satellite receiving has a width θ3dB = 2°• Efficiency of the satellite antenna is η = 0.55 and of the earth station is η = 0.6- power flux density at the satellite is Φ = PtGtmax / 4πR2
- Gain of the earth station is Gtmax =η(πD / λ)2 = 53.1 dBi- Effective isotropic radiated power of earth is EIRP=PtGtmax = 53.1dBi + 20 dBW = 73.1 dBW Then the power flux density is -89.9 dBW/m2
- The power received by the satellite is obtained using the follow equation: Pr= EIRP – attenuation of free space + gain of rx antenna Lfs = 207. 4 dB ; Grmax = η(70π/θ)2 = 6650 = 38.2 dBi with a final value of power
received of -96.1 dBW
Winter 2002 CS216 - Satellite Networks P08/16
University of California Los AngelesComputer Science Department
Example 2: The downlink
• Satellite antenna of Geo fed with Pt = 10 W, that is 10 dBW atfrequency f = 12 GHz
• Beamwidth of 2°
• The same distance of previous example, and the same efficiency forthe satellite and the earth station.
- power flux density at earth station Φ =PtGtmax / 4πR2
- gain of satellite antenna Gtmax = 38.2 dBi and effective isotropic
radiated power EIRP = 10 dBW + 38.2 dBi = 48.2 dBW
with a power flux density of –114.8 dBW/m2
- Lfs = 206.1 dB, Grmax =η( 70π/θ)2 = 151597 = 51.8 dBi
- The power received by antenna of the earth station is obtained using
the same expression of example 1 with a final value of -106.1 dBW