Downlink CNR

Fıgure used in satellite communication systems

Downlink CNR (Carrier to noise ratio in satellite reception) is an important figure in system TVRO design. Below are certain parameters used in CNR computation.

Figure of merit

Figure of merit is given as

f = g t {\displaystyle f={\frac {g}{t}}}

Where t is the temperature and g is the gain of the receiver antenna. For lossless case

t = t a + ( n 1 ) t 0 {\displaystyle t=t_{a}+(n-1)\cdot t_{0}}

and

f = g t a + ( n 1 ) t 0 {\displaystyle f={\frac {g}{t_{a}+(n-1)\cdot t_{0}}}}

where n is the noise factor, ta is the noise temperature of the antenna and t0 is the temperature of the environment (taken as 2900K). F in db is simply

F = 10   log 10 ( f ) {\displaystyle F=10\ \log _{10}(f)}

Path loss

Path loss is defined as

l = ( 4 π d λ ) 2 {\displaystyle l=({\frac {4\cdot \pi \cdot d}{\lambda }})^{2}}

Where λ {\displaystyle \lambda } is the wavelength of the carrier and the d is the distance in meters between the satellite and the receiver . For Geosynchronous satellites this distance is 35,786 kilometres (22,236 mi) at the projection on the earth (at the mean sea level). In actual cases the distance is slightly more than this figure depending on the geographic location. (But for geosynchronous satellites the variation is less than 1%). The Path loss in dB is

L = 20   log 10 ( 4 π d λ ) {\displaystyle L=20\ \log _{10}\left({\frac {4\cdot \pi \cdot d}{\lambda }}\right)}

The same relation can be given in terms of frequency.

L = 20   log 10 ( 4 π d f c ) {\displaystyle L=20\ \log _{10}\left({\frac {4\cdot \pi \cdot d\cdot f}{c}}\right)}

Where c is the velocity of light.

With metric units

L = 147.56 + 20   log 10 ( d ) + 20   log 10 ( f ) {\displaystyle L=-147.56+20\ \log _{10}(d)+20\ \log _{10}(f)}

Using km for d and GHz for f

L = 92.45 + 20   log 10 ( d ) + 20   log 10 ( f ) {\displaystyle L=92.45+20\ \log _{10}(d)+20\ \log _{10}(f)}

Using miles for d and GHz for f

L = 96.58 + 20   log 10 ( d ) + 20   log 10 ( f ) {\displaystyle L=96.58+20\ \log _{10}(d)+20\ \log _{10}(f)}

[1][2]

EIRP

Pe is the Equivalent isotropically radiated power (also known as EIRP) in dBW. It depends on the output of the transponders of the satellite and the antenna gain of the transmitting antenna. This figure is given by the service provider.

P e = 10   log 10 ( p ) + 10   log 10 ( g t ) {\displaystyle P_{e}=10\ \log _{10}(p)+10\ \log _{10}(g_{t})}

where p is the output power of the transponder and g is the antenna gain.

Baseband

B is the baseband of the channel given in dB

B = 10   log 10 ( b ) {\displaystyle B=10\ \log _{10}(b)}

Where b is the base band given in metric units (Hz).

When b is given in MHz, than

B = 10   log 10 ( b ) + 60 {\displaystyle B=10\ \log _{10}(b)+60}

Boltzmann constant

K is the Boltzmann constant given in dB units.

K = 10   log 10 ( 1.380 10 23 ) = 228.6 {\displaystyle K=10\ \log _{10}(1.380\cdot 10^{-23})=-228.6}

CNR in dB units

CNR = f i g u r e o f m e r i t + E I R P f r e e s p a c e p a t h l o s s + 228.6 {\textstyle {\mbox{CNR}}=figureofmerit+EIRP-freespacepathloss+228.6}

References

  1. ^ Reference Data for radio Engineers , Howard W.sams Co.ISBN 0-672-21218-8, p.33-3
  2. ^ Elektrik Mühendisliği No 257, Haşmet Esen : Uydulardan Doğrudan yayın, Ankara,141-152
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