EXPERIMENTAL CORRELATION OF SOOT SPECTRAL ABSORPTION COEFFICIENT

A relatively simple empirical relation for the absorption coefficient kλ, found experimentally in some instances, is

 

                                                         (D-3)

 

where C is the soot volume concentration (volume of particles per unit volume of cloud), and k is a constant. The λ is in μm for the numerical quantities given here. Hottel (1954) recommends using

 

                                                        (D-4)

 

for λ > 0.8 μm. In some experiments, Siddall and McGrath (1963) also found the functional relation of (D-4) to hold approximately. They give, in the range λ = 1-7 μm, the following mean values of α:

Source of soot

Mean α for λ = 1–7 μm

Amyl acetate

0.89, 1.04

Avtur kerosene

0.77

Benzene

0.94, 0.95

Candle

0.93

Furnace samples

0.96, 1.14, 1.25

Petrotherm

1.06

Propane

1.00

 

In Köylü and Faeth (1996) the extinction by soot was examined for acetylene, propylene, ethylene, and propane. The exponent was found as α = 0.83 ± 0.08 for all of these fuels. This was reasonable for the spectral range λ = 0.514–5.2 μm.

 

In Siddall and McGrath (1963) the data were inspected in more detail to see whether α had a functional variation with λ that would provide a more accurate correlation than using a constant α. In some instances α took the form

 

 

where c1 and c2 are positive constants. Examples are in Fig D-1. In other cases, a more general polynomial was required to express α as a function of λ, Fig. D-2. Thus, as a generalization of (D-4) for the infrared region,

 

                                                               (D-5)

 

and letting α be a constant is only an approximation.

A006x010

FIGURE D-1 Experimental values of the exponent a plotted against l for cases where a varies approximately linearly with ln l [Siddall and McGrath (1963)].

 

A006x011

FIGURE D-2 Experimental values of the exponent a plotted against l for cases where a does not vary linearly with ln l [Siddall and McGrath (1963)].

 

 

In the visible range experimental data led to the recommended form [Hottel (1954)]

 

                                                             (D-6)

 

for the wavelength region around λ = 0.6 μm (λ ≈ 0.3 – 0.8 μm).