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1
6.6.
LINK BUDGETLINK BUDGET
PERFORMANCEPERFORMANCE
• characteristics of
– TX station
– RX station
• propagation
• noise, interference
• characteristics of satellite
2
NOISENOISE
• noise voltage
• independent of frequency, “white” noise
kTBRun 4
2

k = 1.38 10-23 J/K, Boltzmann constant
B... noise bandwidth
R...resistance
T...absolute temperature
NOISENOISE
• at very high frequencies thermal noise
vanishes, only quantum noise remains
• Noise power
kTBBNN  0
3
INVERSE SQUARE LAWINVERSE SQUARE LAW
• Carrier power
• Aeff... effective antenna aperture
• R...distance
• GT...transmit antenna gain
AG
R
PC effT
T
2
4

ANTENNA FORMULAANTENNA FORMULA
• effective aperture
A
G
Aeff 
4
2
2
222
2
4
4 DDG 
4
CARRIER POWERCARRIER POWER







44
2
2
G
R
GP
C RTT
GPEIRP TT






R
Ls
4
2
free-space loss
CARRIER/NOISE RATIOCARRIER/NOISE RATIO
BTk
N
C
N
N
C
C s
  kBT
G
R
GP
N
C
s
RTT 1
/4
2 






  kT
G
R
GP
N
C
s
RTT
o
1
/4
2 






5
FIGURE OF MERITFIGURE OF MERIT
• G/T
• important characteristic for
– satellite
– ground station
LINK BUDGETLINK BUDGET
CALCULATIONCALCULATION
• figures may vary widely
– EIRP high
– free-space loss very high
– receive carrier power very low
• logarithmic representation
advantageous
6
LOGARITHMICLOGARITHMIC
REPRESENTATIONREPRESENTATION
• Signal-to-noise ratio [dB]
 
)log(10)log(10)log(10
)log(10/4log20)log(10)log(10
BkT
GRGP
N
C
s
RTT


  BkTGLEIRP dBHzKdBJKdBdBsdBW
N
C
][]/[]/[][][ / 
C/NC/Noo
• carrier power / noise density
  kTGLEIRP KdBJKdBdBsdBW
oN
C
]/[]/[][][ / 
7
C/TC/T
• sometimes used in link budgets
• in [dBW/K]
• leaves out k = -228.6 dB(J/K)
• at the end of calculation B, k considered
 TGLEIRP KdBdBsdBW
T
C
/ ]/[][][

EEbb/N/Noo
• energy per bit / noise density
• r...rate of information rate (not
necessarily channel rate)
r
B
N
C
N
E
o
b

8
SHANNON BOUNDSHANNON BOUND







N
C
BH 1log2
)/1(log/)/1(log
/
22 BNoCNoCBNoCH
CBNB o

eNCH o
B
log/lim 2


SHANNON BOUNDSHANNON BOUND
• limiting case: transmission rate = H:
e
N
HEH b
log2
0

dB
N
E
o
b
6.1
9
EXAMPLEEXAMPLE
• EIRP
– f = 14.0 GHz
– antenna diameter: 2.4 m
– antenna efficiency: 60%
– transmit power: 16 W
dB
E
E
D
G 7.48
914
83
4.2
6.0log10log10 2
22
2
22




























EXAMPLE (2)EXAMPLE (2)
• corresponds to 1,174,897.5 W
dBWEIRP 7.607.48)16log(10 
10
EXAMPLE (3)EXAMPLE (3)
• free-space loss
• f = 14 GHz












 





0214.0
6394
log20
4
log20log10
4
2
ERR
Ls
= 207.2 dB
EXAMPLE (4)EXAMPLE (4)
• free-space loss
• f = 11 GHz












 





0272.0
6394
log20
4
log20log10
4
2
ERR
Ls
= 205 dB
11
EXAMPLE (5)EXAMPLE (5)
• free-space loss
• f = 30 GHz












 





01.0
6394
log20
4
log20log10
4
2
ERR
Ls
= 213.8 dB
ANTENNA GAINANTENNA GAIN
• 14 GHz: G = 48.7 dB
• 30 GHz: G = 55.3 dB
• difference: + 6.6 dB
• difference in free-space loss: - 6.6 dB !
12
C/NC/N
• f = 14.0 GHz
• GT= 48.7 dB
• P = 16 W = 12 dBW
• R = 39,000,000 m
• G/T = 4.2 dB/K
• B = 1 MHz
  BkTGLEIRP dBHzKdBJKdBdBsdBW
N
C
][]/[]/[][][ / 
dB
N
C
3.260.60)6.228(2.42.2077.60
0

C/NC/Noo
• normalized to 1 Hz noise bandwidth
dBHz
N
C
3.86)6.228(2.42.2077.60
0

13
C/TC/T
• without k
KdBW
T
C
/3.1422.42.2077.60 
BACK-OFFBACK-OFF
• usually the max. EIRP of ground station
is given
• back-off in dB from max. EIRP
• EIRP = EIRPmax - BO
• max. EIRP may drive HPA into
saturation
– not possible for multi-carrier operation
– also degradation depending on modulation
scheme
14
ADDITIONAL LOSSESADDITIONAL LOSSES
OUTPUT LOSSESOUTPUT LOSSES
• HPA connected to feed via waveguide
• resulting in additional loss
• design should be such that output
losses are minimum
• Lout
15
POINTING LOSSPOINTING LOSS
• antennas not totally aligned
• movement of satellite
• pointing loss,
• 0.2...1 dB
• Lpu
CONTOUR LOSSCONTOUR LOSS
• satellite antenna gain reduces at outer
zones with respect to beam center
G/T = 4.2 dB/K
G/T = 0.2 dB/K
16
ATMOSPHERICATMOSPHERIC
ATTENUATIONATTENUATION
• gaseous absorption in atmosphere
• attenuation by hydrometeors
• depending on rain rate, drop size,
frequency
• Latu
C/T at TRANSPONDERC/T at TRANSPONDER
 TGLLLLLBOEIRP
T
C
atucupuout su / 
17
EXAMPLEEXAMPLE
• f = 14.0 GHz
• GT= 48.7 dB
• P = 16 W = 12 dBW
• Output back-off: 2 dB
• R = 39,000,000 m
• G/T = 4.2 dB/K
EXAMPLEEXAMPLE
• Lout = 0.7 dB
• Latu = 0.6 dB
• Lcu = 3 dB
• Lpu = 0.4 dB
18
RESULTRESULT
 TGLLLLLBOEIRP
T
C
atucupuout su / 
KdBW
T
C
/3.1482.46.034.02.20727.60 
POWER FLUX DENSITYPOWER FLUX DENSITY
• At transponder input
r
EIRP
A
EIRP effeff
2
4

LLLL
GP
EIRP
atucuout pu
Tout
eff 
LLLLGPEIRP atupucuoutTouteff 
in dB
19
SPREADING LOSSSPREADING LOSS
)4log(10 2
rLspr  in dBm 2
mdBLspr
22
8.162)390000004log(10 
INPUT FLUX DENSITYINPUT FLUX DENSITY
• in dBW/m2
LLLLLGP spratupucuoutTout 
20
TRANSPONDER FLUXTRANSPONDER FLUX
DENSITYDENSITY
• parameter of transponder
• IPFD… input power flux density for
saturation
• can be set by telemetry to adjust the
sensitivity of transponder
• e.g. sat = - 98 dBW/m2
INPUT BACK-OFFINPUT BACK-OFF
• Difference of actual received flux
density and IPFD
• Bin = sat - 
21
POWER TRANSFER CURVEPOWER TRANSFER CURVE
Input back-off
Output
back-off
sat
Bin
Bout
EXAMPLEEXAMPLE
• Pout = 16 W = 12 dBW
• GT = 46.3 dB
• Output loss: 0.7 dB
• Distance R = 39,000 km (24,375 mi)
• Pointing loss: 0.3 dB
• Contour: 1 dB
• Atmospheric attenuation: 1.5 dB
22
EXAMPLE (EXAMPLE (contcont.).)
mdBLspr
22
8.162)390000004log(10 
LLLLLGP spratupucuoutTout 
8.1625.13.017.03.4812 
mdBW 2
/106
EXAMPLE (EXAMPLE (contcont.).)
sat = -98 dBW/m2
• Bin = sat - dB
23
Input back-off
Output
back-off
sat
Bin= 8 dB
Bout= 3.5 dB
in linear region: Bout = Bin - 4.5 dB typically
SATELLITE EIRPSATELLITE EIRP
• Maximum EIRP of transponder:
specified EIRPsat
• EIRP due to drive level:
EIRP = EIRPsat - Bout
• Example:
• EIRPsat = 49 dBW
EIRP = 49 - 3.5 = 45.5 dBW

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Link budget

  • 1. 1 6.6. LINK BUDGETLINK BUDGET PERFORMANCEPERFORMANCE • characteristics of – TX station – RX station • propagation • noise, interference • characteristics of satellite
  • 2. 2 NOISENOISE • noise voltage • independent of frequency, “white” noise kTBRun 4 2  k = 1.38 10-23 J/K, Boltzmann constant B... noise bandwidth R...resistance T...absolute temperature NOISENOISE • at very high frequencies thermal noise vanishes, only quantum noise remains • Noise power kTBBNN  0
  • 3. 3 INVERSE SQUARE LAWINVERSE SQUARE LAW • Carrier power • Aeff... effective antenna aperture • R...distance • GT...transmit antenna gain AG R PC effT T 2 4  ANTENNA FORMULAANTENNA FORMULA • effective aperture A G Aeff  4 2 2 222 2 4 4 DDG 
  • 4. 4 CARRIER POWERCARRIER POWER        44 2 2 G R GP C RTT GPEIRP TT       R Ls 4 2 free-space loss CARRIER/NOISE RATIOCARRIER/NOISE RATIO BTk N C N N C C s   kBT G R GP N C s RTT 1 /4 2          kT G R GP N C s RTT o 1 /4 2       
  • 5. 5 FIGURE OF MERITFIGURE OF MERIT • G/T • important characteristic for – satellite – ground station LINK BUDGETLINK BUDGET CALCULATIONCALCULATION • figures may vary widely – EIRP high – free-space loss very high – receive carrier power very low • logarithmic representation advantageous
  • 6. 6 LOGARITHMICLOGARITHMIC REPRESENTATIONREPRESENTATION • Signal-to-noise ratio [dB]   )log(10)log(10)log(10 )log(10/4log20)log(10)log(10 BkT GRGP N C s RTT     BkTGLEIRP dBHzKdBJKdBdBsdBW N C ][]/[]/[][][ /  C/NC/Noo • carrier power / noise density   kTGLEIRP KdBJKdBdBsdBW oN C ]/[]/[][][ / 
  • 7. 7 C/TC/T • sometimes used in link budgets • in [dBW/K] • leaves out k = -228.6 dB(J/K) • at the end of calculation B, k considered  TGLEIRP KdBdBsdBW T C / ]/[][][  EEbb/N/Noo • energy per bit / noise density • r...rate of information rate (not necessarily channel rate) r B N C N E o b 
  • 8. 8 SHANNON BOUNDSHANNON BOUND        N C BH 1log2 )/1(log/)/1(log / 22 BNoCNoCBNoCH CBNB o  eNCH o B log/lim 2   SHANNON BOUNDSHANNON BOUND • limiting case: transmission rate = H: e N HEH b log2 0  dB N E o b 6.1
  • 9. 9 EXAMPLEEXAMPLE • EIRP – f = 14.0 GHz – antenna diameter: 2.4 m – antenna efficiency: 60% – transmit power: 16 W dB E E D G 7.48 914 83 4.2 6.0log10log10 2 22 2 22                             EXAMPLE (2)EXAMPLE (2) • corresponds to 1,174,897.5 W dBWEIRP 7.607.48)16log(10 
  • 10. 10 EXAMPLE (3)EXAMPLE (3) • free-space loss • f = 14 GHz                    0214.0 6394 log20 4 log20log10 4 2 ERR Ls = 207.2 dB EXAMPLE (4)EXAMPLE (4) • free-space loss • f = 11 GHz                    0272.0 6394 log20 4 log20log10 4 2 ERR Ls = 205 dB
  • 11. 11 EXAMPLE (5)EXAMPLE (5) • free-space loss • f = 30 GHz                    01.0 6394 log20 4 log20log10 4 2 ERR Ls = 213.8 dB ANTENNA GAINANTENNA GAIN • 14 GHz: G = 48.7 dB • 30 GHz: G = 55.3 dB • difference: + 6.6 dB • difference in free-space loss: - 6.6 dB !
  • 12. 12 C/NC/N • f = 14.0 GHz • GT= 48.7 dB • P = 16 W = 12 dBW • R = 39,000,000 m • G/T = 4.2 dB/K • B = 1 MHz   BkTGLEIRP dBHzKdBJKdBdBsdBW N C ][]/[]/[][][ /  dB N C 3.260.60)6.228(2.42.2077.60 0  C/NC/Noo • normalized to 1 Hz noise bandwidth dBHz N C 3.86)6.228(2.42.2077.60 0 
  • 13. 13 C/TC/T • without k KdBW T C /3.1422.42.2077.60  BACK-OFFBACK-OFF • usually the max. EIRP of ground station is given • back-off in dB from max. EIRP • EIRP = EIRPmax - BO • max. EIRP may drive HPA into saturation – not possible for multi-carrier operation – also degradation depending on modulation scheme
  • 14. 14 ADDITIONAL LOSSESADDITIONAL LOSSES OUTPUT LOSSESOUTPUT LOSSES • HPA connected to feed via waveguide • resulting in additional loss • design should be such that output losses are minimum • Lout
  • 15. 15 POINTING LOSSPOINTING LOSS • antennas not totally aligned • movement of satellite • pointing loss, • 0.2...1 dB • Lpu CONTOUR LOSSCONTOUR LOSS • satellite antenna gain reduces at outer zones with respect to beam center G/T = 4.2 dB/K G/T = 0.2 dB/K
  • 16. 16 ATMOSPHERICATMOSPHERIC ATTENUATIONATTENUATION • gaseous absorption in atmosphere • attenuation by hydrometeors • depending on rain rate, drop size, frequency • Latu C/T at TRANSPONDERC/T at TRANSPONDER  TGLLLLLBOEIRP T C atucupuout su / 
  • 17. 17 EXAMPLEEXAMPLE • f = 14.0 GHz • GT= 48.7 dB • P = 16 W = 12 dBW • Output back-off: 2 dB • R = 39,000,000 m • G/T = 4.2 dB/K EXAMPLEEXAMPLE • Lout = 0.7 dB • Latu = 0.6 dB • Lcu = 3 dB • Lpu = 0.4 dB
  • 18. 18 RESULTRESULT  TGLLLLLBOEIRP T C atucupuout su /  KdBW T C /3.1482.46.034.02.20727.60  POWER FLUX DENSITYPOWER FLUX DENSITY • At transponder input r EIRP A EIRP effeff 2 4  LLLL GP EIRP atucuout pu Tout eff  LLLLGPEIRP atupucuoutTouteff  in dB
  • 19. 19 SPREADING LOSSSPREADING LOSS )4log(10 2 rLspr  in dBm 2 mdBLspr 22 8.162)390000004log(10  INPUT FLUX DENSITYINPUT FLUX DENSITY • in dBW/m2 LLLLLGP spratupucuoutTout 
  • 20. 20 TRANSPONDER FLUXTRANSPONDER FLUX DENSITYDENSITY • parameter of transponder • IPFD… input power flux density for saturation • can be set by telemetry to adjust the sensitivity of transponder • e.g. sat = - 98 dBW/m2 INPUT BACK-OFFINPUT BACK-OFF • Difference of actual received flux density and IPFD • Bin = sat - 
  • 21. 21 POWER TRANSFER CURVEPOWER TRANSFER CURVE Input back-off Output back-off sat Bin Bout EXAMPLEEXAMPLE • Pout = 16 W = 12 dBW • GT = 46.3 dB • Output loss: 0.7 dB • Distance R = 39,000 km (24,375 mi) • Pointing loss: 0.3 dB • Contour: 1 dB • Atmospheric attenuation: 1.5 dB
  • 22. 22 EXAMPLE (EXAMPLE (contcont.).) mdBLspr 22 8.162)390000004log(10  LLLLLGP spratupucuoutTout  8.1625.13.017.03.4812  mdBW 2 /106 EXAMPLE (EXAMPLE (contcont.).) sat = -98 dBW/m2 • Bin = sat - dB
  • 23. 23 Input back-off Output back-off sat Bin= 8 dB Bout= 3.5 dB in linear region: Bout = Bin - 4.5 dB typically SATELLITE EIRPSATELLITE EIRP • Maximum EIRP of transponder: specified EIRPsat • EIRP due to drive level: EIRP = EIRPsat - Bout • Example: • EIRPsat = 49 dBW EIRP = 49 - 3.5 = 45.5 dBW