1. Satellite Link Design
Joe Montana
IT Fall 2003

2. Agenda Basic Transmission Theory Review of Decibel Link Budget
System Noise Power (Part 1)

3. Basic Transmission Theory

4. Link Budget parameters
Transmitter power at the antenna
Antenna gain compared to isotropic radiator
EIRP
Flux density at receiver
Free space path loss
System noise temperature
Figure of merit for receiving system
Carrier to thermal noise ratio
Carrier to noise density ratio
Carrier to noise ratio

5. Isotropic Radiator W/m2
Consider an Isotropic Source (punctual radiator) radiating Pt Watts uniformly into free space.
At distance R, the area of the spherical shell with center at the source is 4pR2
Flux density at distance R is given by Eq. 4.1
W/m2

6. Isotropic Radiator 2 W/m2 Power Flux Density:
Isotropic Source
Distance R
Pt Watts
Power Flux Density:
Surface Area of sphere = 4pR2
encloses Pt.
W/m2

7. Antenna Gain (Eqn 4.2) sphere = 4p solid radians
We need directive antennas to get power to go in wanted direction.
Define Gain of antenna as increase in power in a given direction compared to isotropic antenna.
(Eqn 4.2)
P() is variation of power with angle.
G() is gain at the direction .
P0 is total power transmitted.
sphere = 4p solid radians

8. Antenna Gain 2
Antenna has gain in every direction! Term gain may be confusing sometimes.
Usually “Gain” denotes the maximum gain of the antenna.
The direction of maximum gain is called “boresight”.

9. The world’s most misused unit ??
Antenna Gain 3
Gain is a ratio:
It is usually expressed in Decibels (dB)
G [dB] = 10 log10 (G ratio)
The world’s most misused unit ??
(we will see more on dBs later)

10. EIRP - 1
An isotropic radiator is an antenna which radiates in all directions equally
Antenna gain is relative to this standard
Antennas are fundamentally passive
No additional power is generated
Gain is realized by focusing power
Similar to the difference between a lantern and a flashlight
Effective Isotropic Radiated Power (EIRP) is the amount of power the transmitter would have to produce if it was radiating to all directions equally
Note that EIRP may vary as a function of direction because of changes in the antenna gain vs. angle

11. EIRP - 2 The output power of a transmitter HPA is: Pout watts
Some power is lost before the antenna:
Pt =Pout /Lt watts reaches the antenna
Pt = Power into antenna
The antenna has a gain of:
Gt relative to an isotropic radiator
This gives an effective isotropic radiated power of:
EIRP = Pt Gt watts relative to a 1 watt isotropic radiator
HPA
Pout Lt Pt
EIRP

12. Power Flux Density - 1
We now want to find the power density at the receiver
We know that power is conserved in a lossless medium
The power radiated from a transmitter must pass through a spherical shell on the surface of which is the receiver
The area of this spherical shell is 4pR2
Therefore spherical spreading loss is 1/4pR2

13. Power Flux Density - 2
Power flux density (p.f.d.) is a measure of the power per unit area
This is a regulated parameter of the system
CCIR regulations limit the p.f.d. of any satellite system
CCIR regulations are enforced by signatory nations
Allowable p.f.d. varies w.r.t. elevation angle
Allows control of interference
Increasing importance with proliferation of LEO systems

14. Received Power
We can rewrite the power flux density now considering the transmit antenna gain:
(Eqn. 4.3)
The power available to a receive antenna of area Ar m2 we get:
(Eqs. 4.4, 4.6)

15. Effective Aperture
Real antennas have effective flux collecting areas which are LESS than the physical aperture area.
Define Effective Aperture Area Ae:
(Eqn. 4.5)
Where Aphy is actual (physical) aperture area.
Very good: 75%
Typical: 55%
 = aperture efficiency

16. Effective Aperture - 2
Antennas have (maximum) gain G related to the effective aperture area as follows:
Where:
Ae is effective aperture area.

17. Aperture Antennas
Aperture antennas (horns and reflectors) have a physical collecting area that can be easily calculated from their dimensions:
Therefore, using Eqn. 4.7 and Eqn. 4.5 we can obtain the formula for aperture antenna gain as:
Typical values of :
Reflectors: 50-60%
Horns: %

18. Aperture Antenna Types
HORN
Efficient, Low Gain, Wide Beam
REFLECTOR
High Gain, Narrow Beam, May have to be deployed in space
Let’s concentrate on the REFLECTORS in the next slides

19. Symmetrical, Front-Fed
Reflector Types
Symmetrical, Front-Fed
Offset, Front-Fed
Offset-Fed, Cassegranian
Offset-Fed, Gregorian

20. Reflector Antenna -1
A rule of thumb to calculate a reflector antenna beamwidth in a given plane as a function of the antenna dimension in that plane is given by:
degrees
(Eqn. 3.2)
The approximation above, together with the definition of gain (previous page) allow a gain approximation (for reflectors only):
Assuming for instance a typical aperture efficiency of 0.55 gives:

21. Antenna Beamwidth Peak (i.e. maximum) GAIN
Angle between the 3 dB down points is the beamwidth of the antenna

22. Back to Received Power…
The power available to a receive antenna of effective area Ar = Ae m2 is:
(Eqn. 4.6)
Where Ar = receive antenna effective aperture area = Ae
Inverting the equation given for gain (Eq. 4.7) gives:
Inverting…

23. Back to Received Power…
Substituting in Eqn. 4.6 gives:
Friis Transmission Formula
(Eqn. 4.8)
The inverse of the term at the right referred to as “Path Loss”, also known as “Free Space Loss” (Lp):
Therefore…

24. More complete formulation
Demonstrated formula assumes idealized case.
Free Space Loss (Lp) represents spherical spreading only.
Other effects need to be accounted for in the transmission equation:
La = Losses due to attenuation in atmosphere
Lta = Losses associated with transmitting antenna
Lra = Losses associates with receiving antenna
Lpol = Losses due to polarization mismatch
Lother = (any other known loss - as much detail as available)
Lr = additional Losses at receiver (after receiving antenna)

25. Transmission Formula
Some intermediate variables were also defined before:
Pt =Pout /Lt EIRP = Pt Gt
Where:
Pt = Power into antenna
Lt = Loss between power source and antenna
EIRP = effective isotropic radiated power
Therefore, there are many ways the formula could be rewritten. The user has to pick the one most suitable to each need.

26. Link Power Budget Tx Rx EIRP Transmission: HPA Power
Transmission Losses
(cables & connectors)
Antenna Gain
Antenna Pointing Loss
Free Space Loss
Atmospheric Loss (gaseous, clouds, rain)
Rx Antenna Pointing Loss
Reception:
Antenna gain
Reception Losses
(cables & connectors)
Noise Temperature Contribution Rx Pr

27. Review of Decibel

28. Why dB?
There is a large dynamic range of parameters in satellite communications
A typical satellite antenna has a gain of >500
Received power flux is about one part in 100,000,000,000,000,000,000 of the transmitted power
Wouldn’t it be nice to have a better way to write these large numbers?
dB also lets many calculations be addition or subtraction!
That’s a lot of zeros!

29. What is a dB?
Decibel (dB) is the unit for 10 times the base 10 logarithmic ratio of two powers
For instance: gain is defined as Pout/Pin (where Pout is usually greater than Pin)
in dB:
Similarly loss is:

30. A Dangerous Calculation in dB!
dB ratios must NEVER be calculated as 20 times the base 10 logarithmic ratio of voltages
Unless of course its more convenient, in which case you must be very, very careful. Here’s why:
If these calculations are performed for say a (passive) transformer with winding ratios of 4 output turns per
input turn, Vout = 4 when Vin = 1. If the last term is
neglected, the gain appears to be G = 20log(4) = 12 dB.
This is a curious result for a passive device!
If the last term is used, Rout = 16 for Rin = 1, so the
last term is -12 dB. This restores the balance at G = 0
as expected for an ideal passive device.
This term is usually forgotten (with tragic results!)

31. Using Decibels - 1 Rules: Multiply A x B: Divide A / B:
(Add dB values)
Divide A / B:
(Subtract dB values)

32. Using Decibels - 2 Rules: Squares: Square roots: (Multiply by 2)
(Divide by 2)

33. Thinking in dB Its useful to be able to think in dB
Note that 18 is 2*3*3.
Since: 2 = 3 dB
and: 3 = 4.8 dB
you can find 18 in dB
in your head by adding
= 12.6
You don’t even need a
calculator!
This is really handy for
checking link budgets
quickly.

34. References in dB dB values can be referenced to a standard
The standard is simply appended to dB
Typical examples are:

35. Link Budget

36. Translating to dBs The transmission formula can be written in dB as:
This form of the equation is easily handled as a spreadsheet (additions and subtractions!!)
The calculation of received signal based on transmitted power and all losses and gains involved until the receiver is called “Link Power Budget”, or “Link Budget”.
The received power Pr is commonly referred to as “Carrier Power”, C.

37. Link Power Budget Now all factors are accounted for Tx
as additions and subtractions Tx
EIRP
Transmission:
+ HPA Power
Transmission Losses
(cables & connectors)
+ Antenna Gain
Antenna Pointing Loss
Free Space Loss
Atmospheric Loss (gaseous, clouds, rain)
- Rx Antenna Pointing Loss
Reception:
+ Antenna gain
Reception Losses
(cables & connectors)
+ Noise Temperature Contribution Rx Pr

38. 4 Easy Steps to a Good Link Power Budget
First, draw a sketch of the link path
Doesn’t have to be artistic quality
Helps you find the stuff you might forget
Next, think carefully about the system of interest
Include all significant effects in the link power budget
Note and justify which common effects are insignificant here
Roll-up large sections of the link power budget
Ie.: TXd power, TX ant. gain, Path loss, RX ant. gain, RX losses
Show all components for these calculations in the detailed budget
Use the rolled-up results in build a link overview
Comment the link budget
Always, always, always use units on parameters (dBi, W, Hz ...)
Describe any unusual elements (eg. loss caused by H20 on radome)

39. Simple Link Power Budget

40. Why calculate Link Budgets?
System performance tied to operation thresholds.
Operation thresholds Cmin tell the minimum power that should be received at the demodulator in order for communications to work properly.
Operation thresholds depend on:
Modulation scheme being used.
Desired communication quality.
Coding gain.
Additional overheads.
Channel Bandwidth.
Thermal Noise power.
We will see more on
these items in the
next classes.

41. Closing the Link
We need to calculate the Link Budget in order to verify if we are “closing the link”.
Pr >= Cmin  Link Closed
Pr < Cmin  Link not closed
Usually, we obtain the “Link Margin”, which tells how tight we are in closing the link:
Margin = Pr – Cmin
Equivalently:
Margin > 0  Link Closed
Margin < 0  Link not closed

42. Carrier to Noise Ratios
C/N: carrier/noise power in RX BW (dB)
Allows simple calculation of margin if:
Receiver bandwidth is known
Required C/N is known for desired signal type
C/No: carrier/noise p.s.d. (dbHz)
Allows simple calculation of allowable RX bandwidth if required C/N is known for desired signal type
Critical for calculations involving carrier recovery loop performance calculations

43. System Figure of Merit G/Ts: RX antenna gain/system temperature
Also called the System Figure of Merit, G/Ts
Easily describes the sensitivity of a receive system
Must be used with caution:
Some (most) vendors measure G/Ts under ideal conditions only
G/Ts degrades for most systems when rain loss increases
This is caused by the increase in the sky noise component
This is in addition to the loss of received power flux density

44. System Noise Power

45. System Noise Power - 1
Performance of system is determined by C/N ratio.
Most systems require C/N > 10 dB.
(Remember, in dBs: C - N > 10 dB)
Hence usually: C > N dB
We need to know the noise temperature of our receiver so that we can calculate N, the noise power (N = Pn).
Tn (noise temperature) is in Kelvins (symbol K):

46. We will see more on calculating Ts next class.
System Noise Power - 2
System noise is caused by thermal noise sources
External to RX system
Transmitted noise on link
Scene noise observed by antenna
Internal to RX system
The power available from thermal noise is:
where k = Boltzmann’s constant
= 1.38x10-23 J/K( dBW/HzK),
Ts is the effective system noise temperature, and B is the effective system bandwidth
We will see more on calculating Ts next class.