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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 />

• Model approach is by default stati<strong>on</strong>ary. Modelling of n<strong>on</strong>-stati<strong>on</strong>ary effects requires extensi<strong>on</strong>.<br />

4.3.2 Sum-of-Sinusoids<br />

Example: Jakes’ fading generator, 3GPP SCM<br />

Advantages:<br />

• Correlati<strong>on</strong> across antenna elements <strong>and</strong> time created implicitly.<br />

• N<strong>on</strong>-stati<strong>on</strong>ary processes potentially easier to integrate.<br />

Disadvantages:<br />

• Requires a large number of sinusoids for realistic modelling <strong>and</strong> thus computati<strong>on</strong>ally expensive.<br />

• Resulting Doppler spectra are peaky (with number of peaks less or equal to number of<br />

sinusoids).<br />

• The SOS approach builds <strong>on</strong> the assumpti<strong>on</strong> that any <strong>channel</strong> resp<strong>on</strong>se can be separated into a<br />

sum of reflectors represented as Dirac-functi<strong>on</strong>s in time <strong>and</strong> space.<br />

4.3.3 Problem details<br />

Not all of the above points might be obvious to the reader. In the following, some of the advantages <strong>and</strong><br />

disadvantages are thus explained in more details.<br />

4.3.3.1 Stochastic approach<br />

Filtering process. Essentially, the <strong>channel</strong> resp<strong>on</strong>se is correlated across space <strong>on</strong>ly. This correlati<strong>on</strong> is<br />

characterized by the spatial ACF, which is calculated by numerical integrati<strong>on</strong> from the APS. This spatial<br />

ACF is then mapped into two dimensi<strong>on</strong>s; the correlati<strong>on</strong> between signals at antenna elements depending<br />

<strong>on</strong> inter-element spacing, <strong>and</strong> the correlati<strong>on</strong> between signals in time depending <strong>on</strong> the movement of the<br />

mobile. This yields a two-dimensi<strong>on</strong>al kernel which is then used for filtering uncorrelated Gaussian<br />

samples.<br />

N<strong>on</strong>-stati<strong>on</strong>ary effects. The model is stati<strong>on</strong>ary by default. While the incorporati<strong>on</strong> of certain timevariable<br />

parameters is straightforward, e.g. Ricean K-factor, other n<strong>on</strong>-stati<strong>on</strong>ary effects, i.e. timeevoluti<strong>on</strong><br />

of Doppler spectrum or angle parameters, requires c<strong>on</strong>tinuous re-calculati<strong>on</strong> of the filter kernel<br />

<strong>and</strong> is thus computati<strong>on</strong>ally expensive.<br />

4.3.3.2 SOS approach<br />

Number of sinusoids required. In the SOS framework, fading is ensured by defining the positi<strong>on</strong> of the<br />

sinusoids in delay <strong>and</strong> angle in such a way that a minimum number of sinusoids always falls within the<br />

resoluti<strong>on</strong> capabilities of the observati<strong>on</strong> <strong>system</strong>. This minimum number between 4 <strong>and</strong> 8 [Gald04]<br />

ensures the observati<strong>on</strong> of a close to Rayleigh distributi<strong>on</strong>. If the number of sinusoids drops below this<br />

minimum amount, the observer will first see unusual distributi<strong>on</strong>s <strong>and</strong> finally identify single, discrete<br />

scatterers, both of which is typically not a desired effect. Note that str<strong>on</strong>g discrete scatterers, typically<br />

associated with LOS scenarios, are implemented as an opti<strong>on</strong>al additi<strong>on</strong>al comp<strong>on</strong>ent (SCM secti<strong>on</strong> "Line<br />

of sight") because the power of a single sinusoid is by definiti<strong>on</strong> fixed <strong>and</strong> small (e.g. 1/20 of a tap in<br />

SCM).<br />

In the following, we illustrate this point with an example. In the SOS framework, an APS is generated by<br />

changing the spacing of the sinusoids (because each sinusoid is defined to have equal power). A typical<br />

APS <str<strong>on</strong>g>report</str<strong>on</strong>g>ed for outdoor scenarios is a Laplacian functi<strong>on</strong> with a log-normal distributed AS [AIP02].<br />

Next, we determine how to distribute the sinusoids. The lowest density (sinusoids per degree) occurs at<br />

the outer ends of the Laplacian functi<strong>on</strong> <strong>and</strong> for large AS values (we pick 30 degree according to the<br />

reference). Assuming we want to be accurate to -20dB from the peak of the APS, then the angle range is<br />

roughly ±100 degrees from the centre. Let's say the maximum resoluti<strong>on</strong> of our observer is 10 degree (for<br />

example by using a highly directive antenna). In these 10 degrees we want to have a minimum of say 5<br />

sinusoids, i.e. a density of 5/10. The total required number of sinusoids then can be derived as 2345 per<br />

delay-tap.<br />

There are two ways to decrease this high number of sinusoids. One is the introducti<strong>on</strong> of variability in<br />

power of the sinusoids. The distributi<strong>on</strong> of taps can then be different to the APS <strong>and</strong>, with respect to the<br />

previous example, might be more uniform than Laplacian. Hence, in the limiting case of uniform<br />

distributi<strong>on</strong> of taps, the power at each sinusoid would vary according to the Laplace functi<strong>on</strong>, <strong>and</strong> the<br />

resulting number of sinusoids then would be 101.<br />

The sec<strong>on</strong>d approach for reducing the number of sinusoids is to assume that the AS at each path is not<br />

equal to the total AS (over all paths) but smaller (like in SCM). Following again the example from above<br />

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