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

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Maritime-Mobile Satellite <strong>Propagation</strong> <strong>Effects</strong> 9-7<br />

3<br />

o<br />

BW<br />

≤θ o ≤ . (9-15)<br />

4<br />

• The sea condition is such that the roughness parameter u defined as:<br />

is given by<br />

4π<br />

u = h sin( θo<br />

)<br />

( -16<br />

λ<br />

2 ≤ u 10,<br />

(9-17)<br />

where λ is the wavelength in m, θ o is the elevation angle to the satellite, h0 is the RMS<br />

wave height in m related to the significant wave height H by<br />

ho = H 4 . (9-18)<br />

Employing Figure 9-2, (9-17) implies <strong>for</strong> instance, at 5° elevation<br />

1. 5 H 7.<br />

3 or 0.<br />

4 ho<br />

1.<br />

8 ( m)<br />

≤ ≤<br />

≤ ≤ . (9-19)<br />

Step 2: Find the relative antenna gain Dr (in dB) in the direction <strong>of</strong> the specular reflection<br />

point on the sea. The relative antenna gain is approximately given by<br />

D r<br />

−4<br />

Go<br />

/ 10 2<br />

( ) r<br />

= − 4 × 10 10 −1<br />

θ , (9-20)<br />

where G0 is the antenna gain in dBi (dB above isotropic), <strong>and</strong><br />

θ = 15 . θ<br />

(9-21)<br />

r o<br />

when the beam center is in the direction <strong>of</strong> the satellite. The factor <strong>of</strong> 1.5 (as opposed to<br />

2) is used since a significant portion <strong>of</strong> the multipath energy comes from the region<br />

between the true specular reflection point <strong>and</strong> the horizon [Karasawa <strong>and</strong> Shiokawa,<br />

1984a].<br />

Step 3: Obtain the Fresnel reflection coefficient Rij (in dB), where i represents the<br />

polarization <strong>of</strong> the incident wave <strong>and</strong> j is the polarization <strong>of</strong> the reflected wave. These<br />

reflection coefficients are tabulated <strong>for</strong> the sea at 1.5 GHz in Table 9-1 <strong>for</strong> horizontal<br />

polarization RHH, vertical polarization RVV, <strong>and</strong> circular polarization RCC. The Fresnel<br />

reflection coefficients may also be calculated using the <strong>for</strong>mulas <strong>of</strong> Beckmann <strong>and</strong><br />

Spizzichino [1963].<br />

Step 4: Calculate the correction factor C θ in dB given by<br />

<strong>and</strong><br />

Cθ = 0 dB <strong>for</strong> θo<br />

≥ 7°<br />

(9-22)

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