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Final report on link level and system level channel models - Winner

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WINNER D5.4 v. 1.4<br />

(dB)<br />

XPR H<br />

(dB)<br />

σ<br />

µ<br />

σ<br />

3.4 3.5 1.8 1.8 1.07 0.69 3.3 2.5 3.4 2.3 3.5<br />

10.4 10.0 9.5 6.9<br />

3.4 3.1 2.3 2.8<br />

Notes:<br />

Not<br />

avail.<br />

Not<br />

avail.<br />

Not<br />

avail.<br />

Not<br />

avail.<br />

3.7 5.7 2.3 7.2 7.5<br />

2.5 2.9 0.2 2.8 4.0<br />

1. For scenario B3, XPR H values are not available. In the <strong>channel</strong> model implementati<strong>on</strong>, these<br />

values have been substituted by XPR V .<br />

2. Distributi<strong>on</strong> of XPR is log-normal, i.e., XPR = 10 X/10 , where X is Gaussian with st<strong>and</strong>ard<br />

deviati<strong>on</strong> σ <strong>and</strong> mean µ.<br />

Average powers of the ZDSC are normalized so that the total power of all ZDSCs is equal to <strong>on</strong>e. Then,<br />

the normalized power of the nth ZDSC is<br />

P<br />

'<br />

n<br />

n<br />

= Q<br />

P<br />

∑<br />

n=<br />

1<br />

P<br />

'<br />

n<br />

(3.15)<br />

where Q is the number of ZDSCs. For the case when LOS model is used, the power of the direct<br />

comp<strong>on</strong>ent is c<strong>on</strong>sidered in the normalizati<strong>on</strong> such that the ratio of the direct power to the scattered power<br />

is the K-factor.<br />

'<br />

n<br />

n<br />

=<br />

Q<br />

P<br />

P<br />

( K + 1)∑<br />

n=<br />

1<br />

The K-factor for LOS scenarios can be calculated as given in Table 3.7.<br />

P<br />

'<br />

n<br />

, (3.16)<br />

k<br />

P D<br />

= . (3.17)<br />

k +1<br />

Table 3.7: K factor formulae for LOS scenarios.<br />

Scenarios A1 B1 B3 C1 D1<br />

K [dB] 8.7 + 0.051*d 3+ 0.0142d 6 - 0.26*d 17.1 – 0.021*d 3.7 + 0.019*d<br />

Distance d is in m.<br />

It should be noted that when LOS comp<strong>on</strong>ent exists, the ZDSC will have 10+1 rays.<br />

3.1.3 Directi<strong>on</strong>al distributi<strong>on</strong>s of ZDSCs<br />

There are two types of angle informati<strong>on</strong> for each ZDSC. These are the mean angle <strong>and</strong> the offset angles<br />

of each ray from the mean within each cluster. The zero mean azimuth departure (azimuth arrival) angle<br />

is the transmitter (receiver) broadside directi<strong>on</strong>. The generated mean angle of departures <strong>and</strong> angle of<br />

arrivals are relative to the direct path between transmitter <strong>and</strong> receiver with respect to the broadside of<br />

transmitter or receiver, respectively. The angle definiti<strong>on</strong>s <strong>and</strong> references that are used in the generic<br />

<strong>channel</strong> model are the same as those presented in [3GPP SCM]. The relati<strong>on</strong> between the mean azimuthdeparture<br />

<strong>and</strong> the mean azimuth-arrival probability density functi<strong>on</strong>s of each ZDSC <strong>and</strong> their delays is<br />

generated through correlated large-scale parameters used in the corresp<strong>on</strong>ding density functi<strong>on</strong>s. We<br />

fixed the power azimuth spectrum of each ZDSC at the departure <strong>and</strong> the arrival sides assuming it as<br />

Laplacian. The RMS angle-spread of each ZDSC is fixed to <strong>on</strong>e value, which may be different in<br />

departure from arrival <strong>and</strong> may vary from scenario to scenario. However, the power azimuth spectrum<br />

(PAS) <strong>and</strong> the angle-spread values (AS ) of each ZDSC can be changed in the model if needed. The<br />

distributi<strong>on</strong> parameters of the mean angle of departure (AoD) <strong>and</strong> the mean angle of arrival (AoA) the<br />

ZDSCs may vary from <strong>on</strong>e scenario to another. The ZDSC azimuth-departure PAS <strong>and</strong> azimuth-arrival<br />

PAS are defined by 10 rays having predefined offset angles for Laplacian PAS from the mean angles of<br />

Page 23 (167)

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