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WINNER II pdf - Final Report - Cept

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<strong>WINNER</strong> <strong>II</strong> D1.1.2 V1.1<br />

6.12 Fixed feeder links - Scenario B5<br />

For the stationary feeder scenarios only CDL models have been created. The CDL models are based on<br />

the parameters in the tables below which are derived mostly from literature. Note that the CDL models<br />

only approximate the selected parameters. Basically any antenna pattern can be used with the models<br />

However, for the B5 scenario at distances larger than 300 meters the 3 dB beamwidth γ 3dB of one of the<br />

link ends should be smaller than 10 degrees while the other is smaller than 53 degrees.<br />

6.12.1 Scenario B5a<br />

The clustered delay-line model for the rooftop to rooftop case is given in table below. In stationary<br />

scenarios, i.e. B5, the Doppler shifts of the rays are not a function of the AoAs. Instead, they are obtained<br />

from the movement of the scatterers. In B5 we let one scatterer per cluster be moving while the others are<br />

stationary. The Doppler frequency of the moving scatterers is also included in tables below.<br />

Table 6-18 Parameters selected for scenario B5a LOS stationary feeder: rooftop to rooftop.<br />

Parameter<br />

Power-delay profile<br />

Delay-spread<br />

K-factor<br />

XPR<br />

Doppler<br />

Angle-spread of non-direct components.<br />

Value<br />

Exponential (non-direct paths).<br />

40ns<br />

10dB<br />

30dB<br />

A peak centreed around zero Hz with most energy within<br />

0.1 Hz.<br />

Gaussian distributed clusters with 0.5 degrees intra anglespread.<br />

Composite angle-spread 2 degrees. Same in both<br />

ends.<br />

Table 6-19 LOS Clustered Delay-Line model. Rooftop-to-rooftop.<br />

cluster #<br />

delay<br />

[ns]<br />

Power<br />

[dB]<br />

AoD [º] AoA [º]<br />

Freq. of<br />

one<br />

scatterer<br />

mHz<br />

K-factor<br />

[dB]<br />

XPR = 30dB, MS speed N/A<br />

1 0 -0.39 0.0 0.0 41.6 21.8 -0.42 * -35.2 **<br />

2 10 -20.6 0.9 0.2 -21.5 -33.61<br />

3 20 -26.8 0.3 1.5 -65.2 -39.81<br />

4 50 -24.2 -0.3 2.0 76.2 -37.21<br />

5 90 -15.3 3.9 0.0 10.5 -28.31<br />

6 95 -20.5 -0.8 3.6 -20.2 -33.51<br />

7 100 -28.0 4.2 -0.7 1.3 -41.01<br />

8 180 -18.8 -1.0 4.0 2.2 -31.81<br />

9 205 -21.6 5.5 -2.0 -15.4 -34.61<br />

10 260 -19.9 7.6 -4.1 48.9<br />

*<br />

**<br />

+<br />

Power of dominant ray,<br />

Power of each other ray<br />

Clusters with high K-factor will have 21 rays.<br />

-∞<br />

Number of rays /cluster = 20 +<br />

Ray Power [dB]<br />

-32.91<br />

cluster AS at MS [º] = 0.5<br />

cluster AS at BS [º] = 0.5<br />

Composite AS at MS [º] = 0.76<br />

Composite AS at BS [º] =1.13<br />

Page 72 (82)

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