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Publishers version - DTU Orbit

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Figure 175: (a) Left: Conventions assumed into the integration of the RTE. (b) Right: Conventions<br />

assumed into the integration of the RTE<br />

value Iν(0):<br />

Iν(0) = Iν(s0)exp(−τν(s0))+ 2kν2<br />

c 2<br />

s0<br />

0<br />

αν(s)T(s)exp(−τν(s)ds)ds. (336)<br />

Substituting the equivalent formulation of Iν(s) expressed in Eq. (332) we can rewrite Eq.<br />

(336) as a function of the brightness temperature Tb(s):<br />

Tb(0) = Tb(s0)exp(−τν(s0))+<br />

s0<br />

0<br />

T(s)αν(s)exp(−τν(s))ds, (337)<br />

where Tb(s0)exp(−τν(s0)) is the brightness temperature contribute to the atmosphere from<br />

cosmic background sources attenuated by the optical depth τν(s0) existing between ground<br />

level and the point s0.<br />

Referring to polar axis system of the Figure 175(b), operating the substitution ds =<br />

dz/(cosθ), where θ is angle off zenith axis of the radiometer’s beam (for zenith θ = 0◦ )<br />

and assuming z as the atmosphere layer’s level, the measured ground level brightness temperature<br />

for an upward looking radiometer expressed as function of frequency ν, and elevation<br />

angle θ it will become<br />

Tb(0,ν,θ) Tb(ν,θ) = Tb(∞)exp(−τν(∞))+ 1<br />

cosθ<br />

with the optical depth at z-layer’s quote :<br />

τν(z,θ) = 1<br />

cosθ<br />

z<br />

0<br />

∞<br />

0<br />

T(z)αν(z)exp(−τν(z))dz<br />

(338)<br />

αν(z ′ )dz ′ . (339)<br />

AssumingthecosmicbackgroundcontributeTb(∞)exp(−τ(∞))asnegligiblefortheeffect<br />

of the opacity of the entire atmosphere, we can rewrite Eq. (338) at last as:<br />

∞ <br />

1<br />

Tb(ν,θ) = T(z)<br />

0 cosθ αν(z)exp(−τν(z,θ))<br />

<br />

dz (340)<br />

or:<br />

Tb(ν,θ) =<br />

∞<br />

0<br />

T(z)W(ν,z,θ)dz, (341)<br />

in which the ground level measured brightness temperatures Tb(ν,θ) is expressed as a convolution<br />

integral involving a temperature weighting function<br />

W(ν,z,θ) 1<br />

cosθ αν(z)exp(−τν(z,θ)) (342)<br />

(also defined kernel function) and the thermodynamic temperature profile T(z). From a<br />

physical point of view the brightness temperature Tb(ν,θ) of Eq. (341) can be considered<br />

a “weighted” average over the thermodynamic temperature of the atmosphere along the<br />

integration path<br />

numerically is the integral sum of the elementary emission term T(z)dz from each volume’s element,<br />

264 <strong>DTU</strong> Wind Energy-E-Report-0029(EN)

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