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Propagation Models

FSPL

The fundamental propagation loss occurring between the Tx and Rx antenna is modeled using the standard Free-space Pathloss (FSPL) and Gaseous Absorption Loss (GAL). In a line-of-sight radio system, losses are mainly due to free-space path loss (FSPL). FSPL is proportional to the square of the distance between the transmitter and receiver (spreading loss) as well as the square of the frequency of the radio signal (absorption loss).

FSPLdB=20logd+20logf+92.45FSPL_{dB} = 20\log{d} + 20\log{f} + 92.45

where dd is distance in km and ff is frequency in GHz.

GAL

The Gaseous Absorption Loss models the oxygen absorption loss given by the following equation:

GAL(fc)=α(fc)d/1000GAL(f_{c}) = \alpha(f_{c})d/1000

where,

  • α(fc)\alpha(f_{c}) is frequency dependent oxygen loss [dB/km] characterized in Table 7.6.1-1 in ETSI TR 138 901 V14.0.0, which is shown below.
  • d is the distance in meters.

Figure 6: Frequency dependent oxygen loss

Rain Loss

Rain loss is an important factor in the link level network planning as it affects the overall network availability. It is modeled and included i4n the Terragraph Planner in the following method:

  • Get the value of rain-rate (as R0.01R_{0.01}) from user. This typically ranges from 0 - 120 mm/hr
  • Calculate rain attenuation in dB/km using the following constant values:
k=0.8515,α=0.7486,γR=kR0.01αk = 0.8515, \alpha = 0.7486, \gamma_{R} = kR_{0.01}^\alpha

where,

  • γR\gamma_{R} (in dB/km) is multiplied by distance d to get the attenuation A0.01A_{0.01} [dB] using:

    A0.01=γRdA_{0.01} = \gamma_{R}d
  • A0.01A_{0.01} is used in the link budget calculations in Link Budget Calculations

    If a certain link availability is provided by the user (say pip_{i}, in range 99.9 - 99.999), then A0.01A_{0.01} is adjusted to ApA_{p} using the following set of equations:

    r=min(10.477d0.633R0.010.073αf0.12310.579(1exp(0.024d)),2.5)r = \min(\frac{1}{0.477d^{0.633}R^{0.073\alpha}_{0.01}f^{0.123}-10.579(1-\exp{(0.024d)})}, 2.5) \\
    A0.01=γRdrA_{0.01} = \gamma_{R}dr \\
    ApA0.01=C1p(C2+C3log10p)\frac{A_{p}}{A_{0.01}} = C_{1}p^{-(C_{2}+C_{3}\log_{10}{p})}
    p=100pip = 100 - p_{i}
    C0=0.12+0.4[log10(f/10)0.8]C_{0} = 0.12 + 0.4[\log_{10}{(f/10)^{0.8}}]
    C1=(0.07C0)(0.121C0)C_{1} = (0.07^{C_{0}})(0.12^{1-C_{0}})
    C2=0.855C0+0.546(1C0)C_{2} = 0.855C_{0} + 0.546(1-C_{0})
    C3=0.139C0+0.043(1C0)C_{3} = 0.139C_{0} + 0.043(1-C_{0})