Rotational Raman scattering in the Earth's atmosphere ... - SRON
Rotational Raman scattering in the Earth's atmosphere ... - SRON
Rotational Raman scattering in the Earth's atmosphere ... - SRON
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22 Chapter 2<br />
When layers a and b are <strong>the</strong> same, <strong>the</strong> add<strong>in</strong>g is called doubl<strong>in</strong>g. In this case, <strong>the</strong> number of calculations<br />
can be reduced considerably due to symmetry considerations [de Haan et al., 1987].<br />
To calculate <strong>the</strong> reflection and transmission functions for a homogeneous model layer, <strong>the</strong> doubl<strong>in</strong>g<br />
scheme is applied to a very th<strong>in</strong> sublayer. In general, <strong>the</strong> optical properties of a homogeneous<br />
model layer are characterized by its optical thickness ∆τ, its s<strong>in</strong>gle <strong>scatter<strong>in</strong>g</strong> albedo ω, and its phase<br />
function P . For a very th<strong>in</strong> layer, <strong>the</strong> s<strong>in</strong>gle <strong>scatter<strong>in</strong>g</strong> approximation suffices and yields<br />
{ }<br />
R(ν,µ,ϕ;ν ′ ,µ ′ ,ϕ ′ ) = 1 4 µ ′ ∆τ+µ∆τ 1−e<br />
−∆τ/µ−∆τ ′ /µ ′ ω(ν;ν ′ )P(−µ,ϕ;ν ′ ,µ ′ ,ϕ ′ ) , (2.12)<br />
′<br />
⎧<br />
1 ∆τ ′<br />
e −∆τ/µ ω(ν;ν ′ )P(µ,ϕ;ν ′ ,µ ′ ,ϕ ′ ) if µ ′ ∆τ =µ∆τ ′ ,<br />
4 µ µ<br />
⎪⎨<br />
′<br />
T dif (ν,µ,ϕ;ν ′ ,µ ′ ,ϕ ′ ) = {<br />
1 ∆τ ′<br />
4 µ ⎪⎩<br />
′ ∆τ−µ∆τ e<br />
−∆τ ′ /µ ′ −e −∆τ/µ} (2.13)<br />
ω(ν;ν ′ )P(µ,ϕ;ν ′ ,µ ′ ,ϕ ′ )<br />
′<br />
o<strong>the</strong>rwise .<br />
∆τ ′<br />
Here, ∆τ ′ ≡ ∆τ(ν ′ ) and ∆τ ≡ ∆τ(ν). Fur<strong>the</strong>rmore, we assume that <strong>the</strong> phase function P depends<br />
only on <strong>the</strong> wavenumber of <strong>the</strong> <strong>in</strong>cident light. The <strong>scatter<strong>in</strong>g</strong> probability from wavenumber ν ′ to ν<br />
is given by <strong>the</strong> s<strong>in</strong>gle <strong>scatter<strong>in</strong>g</strong> albedo ω(ν;ν ′ ). Besides R and T dif <strong>in</strong> Eqs.(2.12) and (2.13), which<br />
describe <strong>the</strong> diffuse light, T 0 <strong>in</strong> Eq. (2.5) is used to describe <strong>the</strong> transmission of <strong>the</strong> direct light.<br />
2.3 Numerical implementation<br />
2.3.1 Discretization<br />
In order to implement <strong>the</strong> add<strong>in</strong>g equations (2.6–2.10), a proper discretization of <strong>the</strong> operator product<br />
<strong>in</strong> Eq. (2.11) is required. First of all, <strong>the</strong> dependence on azimuthal angle needs to be circumvented<br />
by represent<strong>in</strong>g <strong>the</strong> reflectivity and transmittance as a Fourier series. In <strong>the</strong> scalar approximation this<br />
is done by expand<strong>in</strong>g <strong>the</strong> reflection and transmission functions as a cos<strong>in</strong>e Fourier series of <strong>the</strong> order<br />
m max ,<br />
R(ν,µ,ϕ;ν ′ ,µ ′ ,ϕ ′ ) =<br />
m∑<br />
max<br />
m=0<br />
R m (ν,µ;ν ′ ,µ ′ ) cos m[ϕ−ϕ ′ ], (2.14)<br />
where R m is <strong>the</strong> mth Fourier component [Liou, 1992]. The add<strong>in</strong>g equations rema<strong>in</strong> valid for each<br />
Fourier component separately (e.g. Hansen and Travis [1974b]).<br />
The <strong>in</strong>tegral over zenith angle <strong>in</strong> <strong>the</strong> operator product <strong>in</strong> Eq. (2.11) can be approximated by a<br />
Gaussian quadrature of order r max with quadrature po<strong>in</strong>ts µ r and weights w r with r = 1,..,r max . In<br />
addition, <strong>the</strong> wavenumber <strong>in</strong>terval ν ∈ [0, ∞] needs to be gridded. We decided to use a f<strong>in</strong>ite 1 cm −1<br />
grid for this purpose, with wavenumber b<strong>in</strong>s ν k and b<strong>in</strong>-widths ∆ν k = 1 cm −1 . This wavenumber<br />
grid seems sufficient for <strong>the</strong> simulation of measurements with a spectral resolution of approximately<br />
0.2 nm.<br />
After a successful discretization, <strong>the</strong> reflection and transmission functions become matrices with<br />
elements [R] m ij;pq, [T ] m ij;pq, [T ∗ ] m ij;pq and [R ∗ ] m ij;pq. The first two <strong>in</strong>dices i and j describe reflection or