Page updated: May 19, 2021
Author: Curtis Mobley
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The Volume Scattering Function (VSF)

We now take into account the angular distribution of the scattered power, with two assumptions. We first assume that the medium is isotropic, i.e., its influence on light is the same in all directions at a given point. This is a reasonable assumption for natural waters in which the particles are randomly oriented by turbulence. We also assume that the incident light is unpolarized. If these two assumptions are true, then the scattering process is azimuthally symmetric. This means that the scattering depends only on the scattering angle ψ, which is measured from the direction of the unscattered beam as shown in Fig. 1. Clearly 0 ψ π.


Figure 1: Geometry used to define the volume scattering function. Φi(λ) is the incident power onto an area ΔA. An amount ΔΦa(λ) of the incident power is absorbed in distance Δr, and Δ2Φ s(ψ,λ) is the power scattered into the annular ring of solid angle ΔΩ. ΔΦt(λ) is the transmitted power.

Conceptual Definition of the Volume Scattering Function

With these two assumptions, the fraction of incident power scattered out of the beam through an angle ψ into a solid angle ΔΩ centered on ψ, is Δ2Φ s(ψ,λ)Φi(λ). The notation Δ2Φ s(ψ,λ) is adopted from ? to indicate that Δ2Φ s(ψ,λ) is a second-order small quantity, that is, it is small because both Δr and ΔΩ are small. The solid angle ΔΩ now includes all directions within the two red rings shown in the figure, corresponding to all directions between scattering angles ψ and ψ + Δψ. The volume scattering function β(ψ,λ) is defined as the limit of this fraction as Δr 0 and ΔΩ 0:

β(ψ,λ) lim Δr0 lim ΔΩ0 Δ2Φ s(ψ,λ) Φi(λ)ΔrΔΩ = 1 Φi(λ) 2Φ s(ψ,λ) rΩ (m1sr1). (1)

Recalling the definition of spectral radiant intensity ?? as scattered power per unit solid angle, the corresponding intensity scattered into the given solid angle ΔΩ is ΔIs(ψ,λ) = Δ2Φ s(ψ,λ)ΔΩ. Moreover, if the incident power Φi(λ) falls on an area ΔA, then the corresponding incident irradiance is Ei(λ) = Φi(λ)ΔA. Noting that ΔV = ΔrΔA is the volume of water that is illuminated by the incident beam allows Eq. (1) to be rewritten as

β(ψ,λ) = lim ΔV 0ΔIs(ψ,λ) Ei(λ)ΔV = 1 Ei(λ) Is(ψ,λ) V . (2)

This form of β(ψ,λ) suggests the name volume scattering function (commonly abbreviated as VSF) and the physical interpretation of scattered intensity per unit incident irradiance per unit volume of water. In the language of a physicist, the VSF also can be interpreted as the differential scattering cross section per unit volume.

The forms of Eqs. (1) and (2) involving partial derivatives are conceptual definitions. Instruments that measure the VSF always have to deal with finite path lengths Δr and finite solid angles ΔΩ. The transition from a definition as a derivative to an instrument design is discussed on Sec. ?? on measuring IOPs.

Scattering Coefficients

Integrating β(ψ,λ) over all directions (solid angles) gives the total scattered power per unit incident irradiance and unit volume of water, in other words the scattering coefficient:

b(λ) =Ξβ(ψ,λ)dΩ = 2π0πβ(ψ,λ) sin ψdψ. (3)

The 2π in the last equation follows from our assumption that the scattering is azimuthally symmetric about the incident direction. This integration is often divided into forward scattering, 0 ψ < π2, and backward scattering, π2 ψ π, parts. The corresponding forward and backward scattering coefficients are, respectively,

bf(λ) 2π0π2β(ψ,λ) sin ψdψ (4)
bb(λ) 2ππ2πβ(ψ,λ) sin ψdψ. (5)

The backscatter fraction, defined by

Bb(λ) = b̃b bb(λ) b(λ) , (6)

gives the fraction of scattered light that is deflected through scattering angles greater than 90 deg. This quantity is fundamental to remote sensing because most of the light leaving the ocean in an upward direction comes from sunlight that was originally heading downward, but which was backscattered into upward directions.

The Scattering Phase Function

The volume scattering phase function1 , β̃(ψ,λ), is defined by

β̃(ψ,λ) β(ψ,λ) b(λ) (sr1). (7)

Writing the VSF β(ψ,λ) as the product of the scattering coefficient b(λ) times the phase function β̃(ψ,λ) partitions β(ψ,λ) into a factor giving the magnitude of the total scattering, b(λ) with units of m1, and a factor giving the angular distribution of the scattered light, β̃(ψ,λ), with units of sr1. Combining Eqs. (3) and (7) gives the normalization condition for the phase function:

2π0πβ̃(ψ,λ) sin ψdψ = 1. (8)

This normalization implies that the backscatter fraction can be computed from

Bb(λ) 2ππ2πβ̃(ψ,λ) sin ψdψ. (9)

The asymmetry parameter g or mean cosine of the phase function is average over all scattering directions of the cosine of the scattering angle ψ, namely

g = cos ψ 2π0πβ̃(ψ) cos ψ sin ψdψ. (10)

The asymmetry parameter is a convenient measure of the “shape” of the phase function. For example, if β̃(ψ) is very large for small ψ, then g is near one. If β̃(ψ) is symmetric about ψ = 90 degrees , then g = 0. Typical ocean waters have g values in the range of 0.8 to 0.95.

Comment: We have assumed above that the scattering is azimuthally symmetric, so that the directional pattern or angular shape of the VSF depends only on the scattering angle ψ. This is not the case for polarized incident light, even if the medium is isotropic. Thus a linearly polarized laser beam will scatter differently for different azimuthal directions (measured relative to the plane of polarization), even if the medium is isotropic. Description of polarized light requires the Stokes vector formalism and a more complicated description of scattering by polarized light; also see The General Vector RTE.

If the medium contains non-spherical particles that are not randomly oriented, even unpolarized light will scatter differently for different azimuthal directions. This is sometimes the case, for example, in cirrus clouds and ice fogs, which can have non-spherical ice crystals that become oriented in a particular way as the crystals fall through a calm atmosphere. The atmosphere is then an optically anisotropic medium, and scattering is not azimuthally symmetric. Scattering of sunlight in such an atmosphere gives rise to phenomena such as “sun dogs” or parhelia, which are bright spots to either side of the sun.

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