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Handbook of Propagation Effects for Vehicular and ... - Courses

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Figure 10-10: Cumulative fade distributions <strong>for</strong> Tokyo, Japan at L-B<strong>and</strong> (1.5 GHz) <strong>for</strong> the<br />

simulated Globalstar constellation. The joint distributions <strong>for</strong> multiple satellites correspond to<br />

“combining diversity.”.............................................................................................................. 10-14<br />

Figure 10-11: Cumulative fade distributions <strong>for</strong> London, Engl<strong>and</strong> at L-B<strong>and</strong> (1.5 GHz) <strong>for</strong> the<br />

simulated Globalstar constellation. The joint distributions <strong>for</strong> multiple satellites correspond to<br />

“combining diversity.”.............................................................................................................. 10-15<br />

Figure 10-12: Cumulative fade distributions <strong>for</strong> Singapore at L-B<strong>and</strong> (1.5 GHz) <strong>for</strong> the simulated<br />

Globalstar constellation. The joint distributions <strong>for</strong> multiple satellites correspond to<br />

“combining diversity.”.............................................................................................................. 10-16<br />

Figure 10-13: Path diversity gains at 1.5 GHz derived from distributions <strong>for</strong> the simulated<br />

Globalstar constellation with “combining” <strong>and</strong> “h<strong>and</strong><strong>of</strong>f” diversity <strong>for</strong> Tokyo, Japan................. 10-16<br />

Figure 10-14: Path diversity gains at 1.5 GHz derived from distributions <strong>for</strong> the simulated<br />

Globalstar constellation with “combining” <strong>and</strong> “h<strong>and</strong><strong>of</strong>f” diversity <strong>for</strong> Singapore...................... 10-17<br />

Table <strong>of</strong> Tables<br />

Table 10-1: Average skyline statistics <strong>for</strong> four locations derived by optical methods. ........................... 10-3<br />

Table 10-2: Parameters associated with lognormal fits associated with histograms <strong>of</strong> the type given<br />

in Figure 10-3<strong>and</strong> percent visibility above 10°. ........................................................................... 10-4<br />

Table 10-3: Fade parameters <strong>of</strong> the three-state fade model................................................................... 10-6<br />

Table 10-4: Tabulation <strong>of</strong> azimuth averaged values <strong>of</strong> C, S <strong>and</strong> B in (10-8) <strong>for</strong> different elevation<br />

angle intervals <strong>for</strong> Tokyo, Japan. ................................................................................................ 10-8<br />

Table 10-5: List <strong>of</strong> values <strong>of</strong> “path-state vector” components C, S, B <strong>for</strong> Globalstar constellation in<br />

London, Tokyo, <strong>and</strong> Singapore. ................................................................................................ 10-10<br />

10-ii

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